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Strengthened African Summer Monsoon in the Mid-Piacenzian


doi: 10.1007/s00376-016-5215-y

  • Using model results from the first phase of the Pliocene Model Intercomparison Project (PlioMIP) and four experiments with CAM4, the intensified African summer monsoon (ASM) in the mid-Piacenzian and corresponding mechanisms are analyzed. The results from PlioMIP show that the ASM intensified and summer precipitation increased in North Africa during the mid-Piacenzian, which can be explained by the increased net energy in the atmospheric column above North Africa. Further experiments with CAM4 indicated that the combined changes in the mid-Piacenzian of atmospheric CO2 concentration and SST, as well as the vegetation change, could have substantially increased the net energy in the atmospheric column over North Africa and further intensified the ASM. The experiments also demonstrated that topography change had a weak effect. Overall, the combined changes of atmospheric CO2 concentration and SST were the most important factor that brought about the intensified ASM in the mid-Piacenzian.
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  • Bonnefille R., 2010: Cenozoic vegetation, climate changes and hominid evolution in tropical Africa. Global and Planetary Change, 72, 390- 411.10.1016/j.gloplacha.2010.01.015159886a23b07c7446bc68b07a331db76http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0921818110000214http://www.sciencedirect.com/science/article/pii/S0921818110000214This paper reviews information on past vegetation of tropical Africa during the Cenozoic, focused upon the last 10 Ma, a time spanning hominid record in Central and East Africa. Summary of palaeobotanical data collected at terrestrial sites are compared with new results on the long term evolution of the continental vegetation zones documented from marine pollen record of two deep sea cores reco...
    Bonnefille R., R. Potts, F. Chaliè D. Jolly, O. Peyron, and T. E. Cerling, 2004: High-resolution vegetation and climate change associated with Pliocene Australopithecus afarensis. Proceedings of the National Academy of Sciences of the United States of America, 101, 12 125- 12 129.10.1073/pnas.0401709101153046557dc7302f576e1d0fd68563fe201567b0http%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpubmed%2F15304655http://med.wanfangdata.com.cn/Paper/Detail/PeriodicalPaper_PM15304655Plio-Pleistocene global climate change is believed to have had an important influence on local habitats and early human evolution in Africa. Responses of hominin lineages to climate change have been difficult to test, however, because this procedure requires well documented evidence for connections between global climate and hominin environment. Through high-resolution pollen data from Hadar, Ethiopia, we show that the hominin Australopithecus afarensis accommodated to substantial environmental variability between 3.4 and 2.9 million years ago. A large biome shift, up to 5 degrees C cooling, and a 200- to 300-mm/yr rainfall increase occurred just before 3.3 million years ago, which is consistent with a global marine delta(18)O isotopic shift.
    Bosmans J. H. C., S. S. Drijfhout, E. Tuenter, L. J. Lourens, F. J. Hilgen, and S. L. Weber, 2012: Monsoonal response to mid-holocene orbital forcing in a high resolution GCM. Climate of the Past, 8, 723- 740.10.5194/cp-8-723-201270cd486f5679b0b0d55842eb302c04f8http%3A%2F%2Fwww.oalib.com%2Fpaper%2F1369438http://www.oalib.com/paper/1369438In this study, we use a sophisticated high-resolution atmosphere-ocean coupled climate model, EC-Earth, to investigate the effect of Mid-Holocene orbital forcing on summer monsoons on both hemispheres. During the Mid-Holocene (6 ka), there was more summer insolation on the Northern Hemisphere than today, which intensified the meridional temperature and pressure gradients. Over North Africa, monsoonal precipitation is intensified through increased landward monsoon winds and moisture advection as well as decreased moisture convergence over the oceans and more convergence over land compared to the pre-industrial simulation. Precipitation also extends further north as the ITCZ shifts northward in response to the stronger poleward gradient of insolation. This increase and poleward extent is stronger than in most previous ocean-atmosphere GCM simulations. In north-westernmost Africa, precipitation extends up to 35° N. Over tropical Africa, internal feedbacks completely overcome the direct warming effect of increased insolation. We also find a weakened African Easterly Jet. Over Asia, monsoonal precipitation during the Mid-Holocene is increased as well, but the response is different than over North-Africa. There is more convection over land at the expense of convection over the ocean, but precipitation does not extend further northward, monsoon winds over the ocean are weaker and the surrounding ocean does not provide more moisture. On the Southern Hemisphere, summer insolation and the poleward insolation gradient were weaker during the Mid-Holocene, resulting in a reduced South American monsoon through decreased monsoon winds and less convection, as well as an equatorward shift in the ITCZ. This study corroborates the findings of paleodata research as well as previous model studies, while giving a more detailed account of Mid-Holocene monsoons.
    Braconnot, P., Coauthors, 2007: Results of PMIP2 coupled simulations of the Mid-Holocene and Last Glacial Maximum-art 2: Feedbacks with emphasis on the location of the ITCZ and mid- and high latitudes heat budget. Climate of the Past, 3, 279- 296.
    Bragg F. J., D. J. Lunt, and A. M. Haywood, 2012: Mid-Pliocene climate modelled using the UK hadley centre model: PlioMIP experiments 1 and 2. Geoscientific Model Development, 5, 1109- 1125.10.5194/gmdd-5-837-2012e2531673d4bd40e05a8d7577b7929ce7http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2156883http://www.oalib.com/paper/2156883The Pliocene Model Intercomparison Project (PlioMIP) project is a sub-project of the Paleoclimate Modelling Intercomparison Project (PMIP) whose objective is to compare predictions of the mid-Pliocene climate from the widest possible range of general circulation models. The mid-Pliocene (3.33.0 Ma) is the most recent sustained period of greater warmth and atmospheric carbon dioxide concentration than the pre-industrial times and as such has potential to inform predictions of our warming climate in the coming century. This paper describes the UK contribution to PlioMIP using the Hadley Centre Model both in atmosphere-only mode (HadAM3, PlioMIP Experiment 1) and atmosphere-ocean coupled mode (HadCM3, PlioMIP Experiment 2). The coupled model predicts a greater overall warming (3.3 °C) relative to the control than the atmosphere-only (2.5 °C). The Northern Hemisphere latitudinal temperature gradient is greater in the coupled model with a warmer equator and colder Arctic than the atmosphere-only model, which is constrained by sea surface temperatures from Pliocene proxy reconstructions. The atmosphere-only model predicts a reduction in equatorial precipitation and south Asian monsoon intensity whereas the coupled models shows and increase in the intensity of these systems. Sensitivity studies using alternative boundary conditions for both the Pliocene and the control simulations are presented, which indicate the sensitivity of the mid-Pliocene warming to uncertainties in both pre-industrial and mid-Pliocene climate.
    Brierley C. M., 2015: Interannual climate variability seen in the Pliocene Model Intercomparison Project. Climate of the Past, 11, 605- 618.10.5194/cp-11-605-2015952d08bc07df7af148df6cfed0933bcdhttp%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2015CliPa..11..605Bhttp://adsabs.harvard.edu/abs/2015CliPa..11..605BFollowing proxy observations of weakened temperature gradients along the Equator in the early Pliocene, there has been much speculation about Pliocene climate variability. A major advance for our knowledge about the later Pliocene has been the coordination of modelling efforts through the Pliocene Model Intercomparison Project (PlioMIP). Here the changes in interannual modes of sea surface temperature variability will be presented across PlioMIP. Previously model ensembles have shown little consensus in the response of the El Niño-Southern Oscillation (ENSO) to imposed forcings - either for the past or future. The PlioMIP ensemble, however, shows surprising agreement with eight models simulating reduced variability and only one model indicating no change. The Pliocene's robustly weaker ENSO also saw a shift to lower frequencies. Model ensembles focussed at a wide variety of forcing scenarios have not yet shown this level of coherency. Nonetheless the PlioMIP ensemble does not show a robust response of either ENSO flavour or sea surface temperature variability in the Tropical Indian and North Pacific Oceans. Existing suggestions of ENSO properties linked to changes in zonal temperature gradient, seasonal cycle and the elevation of the Andes Mountains are investigated, yet prove insufficient to explain the coherent response. The reason for this surprisingly coherent signal warrants further investigation.
    Chan W. L., A. Abe-Ouchi, and R. Ohgaito, 2011: Simulating the mid-Pliocene climate with the MIROC general circulation model: experimental design and initial results. Geoscientific Model Development, 4, 1035- 1049.10.5194/gmd-4-1035-2011897e0a76e17a9eea9db641ab14978fcbhttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F2155458http://www.oalib.com/paper/2155458Recently, PlioMIP (Pliocene Model Intercomparison Project) was established to assess the ability of various climate models to simulate the mid-Pliocene warm period (MPWP), 3.292.97 million years ago. We use MIROC4m, a fully coupled atmosphere-ocean general circulation model (AOGCM), and its atmospheric component alone to simulate the MPWP, utilizing up-to-date data sets designated in PlioMIP as boundary conditions and adhering to the protocols outlined. In this paper, a brief description of the model is given, followed by an explanation of the experimental design and implementation of the boundary conditions, such as topography and sea surface temperature. Initial results show increases of approximately 10 °C in the zonal mean surface air temperature at high latitudes accompanied by a decrease in the equator-to-pole temperature gradient. Temperature in the tropical regions increase more in the AOGCM. However, warming of the AOGCM sea surface in parts of the northern North Atlantic Ocean and Nordic Seas is less than that suggested by proxy data. An investigation of the model-data discrepancies and further model intercomparison studies can lead to a better understanding of the mid-Pliocene climate and of its role in assessing future climate change.
    Chand ler, M., D. Rind, R. Thompson, 1994: Joint investigations of the middle Pliocene climate II: GISS GCM northern hemisphere results. Global and Planetary Change, 9, 197- 219.10.1016/0921-8181(94)90016-7414b69bfee1fb2a57c66fef8acddade6http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2F0921818194900167http://www.sciencedirect.com/science/article/pii/0921818194900167The Pliocene SST pattern implicates increased ocean heat flux as a component force behind the middle Pliocene warmth, since levels of CO 2 , large enough to cause the extreme high latitude temperatures, would generate more tropical warming than is indicated by floral and faunal records. Surface energy fluxes, calculated by the GCM, indicate that an increased meridional ocean heat flux of 32% could reproduce the data-derived SST distribution, despite weakened atmospheric transports. The decreased wind stress valuessuggest that any increase of ocean heat transports would probably have resulted from a strentthening of the thermohaline circulation.
    Chand ler, M. A., L. E. Sohl, J. A. Jonas, H. J. Dowsett, M. Kelley, 2013: Simulations of the mid-Pliocene warm period using two versions of the NASA/GISS ModelE2-R coupled model. Geoscientific Model Development, 6, 517- 531.10.5194/gmd-6-517-201305dbf0080964d16c921edbaffee0dec5http%3A%2F%2Fwww.oalib.com%2Fpaper%2F1377356http://www.oalib.com/paper/1377356The mid-Pliocene Warm Period (mPWP) bears many similarities to aspects of future global warming as projected by the Intergovernmental Panel on Climate Change (IPCC, 2007). Both marine and terrestrial data point to high-latitude temperature amplification, including large decreases in sea ice and land ice, as well as expansion of warmer climate biomes into higher latitudes. Here we present our most recent simulations of the mid-Pliocene climate using the CMIP5 version of the NASA/GISS Earth System Model (ModelE2-R). We describe the substantial impact associated with a recent correction made in the implementation of the Gent-McWilliams ocean mixing scheme (GM), which has a large effect on the simulation of ocean surface temperatures, particularly in the North Atlantic Ocean. The effect of this correction on the Pliocene climate results would not have been easily determined from examining its impact on the preindustrial runs alone, a useful demonstration of how the consequences of code improvements as seen in modern climate control runs do not necessarily portend the impacts in extreme climates. Both the GM-corrected and GM-uncorrected simulations were contributed to the Pliocene Model Intercomparison Project (PlioMIP) Experiment 2. Many findings presented here corroborate results from other PlioMIP multi-model ensemble papers, but we also emphasise features in the ModelE2-R simulations that are unlike the ensemble means. The corrected version yields results that more closely resemble the ocean core data as well as the PRISM3D reconstructions of the mid-Pliocene, especially the dramatic warming in the North Atlantic and Greenland-Iceland-Norwegian Sea, which in the new simulation appears to be far more realistic than previously found with older versions of the GISS model. Our belief is that continued development of key physical routines in the atmospheric model, along with higher resolution and recent corrections to mixing parameterisations in the ocean model, have led to an Earth System Model that will produce more accurate projections of future climate.
    Chou C., J. D. Neelin, 2003: Mechanisms limiting the northward extent of the northern summer monsoons over North America, Asia, and Africa. J.Climate, 16, 406- 425.f963d0d16b102b73ffdf1193ba9fd2e6http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D2003JCli...16..406C%26db_key%3DPHY%26link_type%3DABSTRACThttp://xueshu.baidu.com/s?wd=paperuri%3A%28c78b849ca99a500a08e5bf7e64a1b1be%29&filter=sc_long_sign&tn=SE_xueshusource_2kduw22v&sc_vurl=http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D2003JCli...16..406C%26db_key%3DPHY%26link_type%3DABSTRACT&ie=utf-8&sc_us=1817286737200850422
    Contoux C., G. Ramstein, and A. Jost, 2012: Modelling the mid-Pliocene warm period climate with the IPSL coupled model and its atmospheric component LMDZ5A. Geoscientific Model Development, 5, 903- 917.10.5194/gmdd-5-515-2012adfd166a701b478cdb93fa80070af4d4http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2159393http://www.oalib.com/paper/2159393This paper describes the experimental design and model results of the climate simulations of the mid-Pliocene Warm Period (mPWP, ca. 3.33 Ma) using the Institut Pierre Simon Laplace model (IPSLCM5A), in the framework of the Pliocene Model Intercomparison Project (PlioMIP). We use the IPSL atmosphere ocean general circulation model (AOGCM), and its atmospheric component alone, to simulate the climate of the mPWP. Boundary conditions such as sea surface temperatures (SSTs), topography, ice sheet extent and vegetation are derived from the ones imposed by the Pliocene Model Intercomparison Project (PlioMIP), described in Haywood et al. (2010, 2011). We first describe the IPSL model main features, and then give a full description of the boundary conditions used for atmospheric model and coupled model experiments. The climatic outputs of the mPWP simulations are detailed and compared to the corresponding control simulations. The simulated warming is 1.94 °C in the atmospheric and 1.83 °C in the coupled model experiments. In both experiments, warming is more important at high latitudes. Simulated precipitation has a different behaviour in the coupled model than in the atmospheric model alone, because of the reduced gradients in imposed SSTs, which impacts the Hadley and Walker circulations. In addition, a sensitivity test to the change of land-sea mask in the atmospheric model, representing a sea-level change from present-day to 25 m higher during the mid-Pliocene, is described. We find that surface temperature differences can be important (several degrees Celsius) but are restricted to the areas that were changed from ocean to land or vice versa. In terms of precipitation, there is no impact on polar regions although the change in land-sea mask is important in these areas.
    Cook K. H., G. A. Meehl, and J. M. Arblaster, 2012: Monsoon Regimes and Processes in CCSM4. Part II: African and American Monsoon Systems. J.Climate, 25, 2609- 2621.0b22763d4aef6e339b6ad3fee3e3e077http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D2012JCli...25.2609C%26db_key%3DPHY%26link_type%3DABSTRACThttp://xueshu.baidu.com/s?wd=paperuri%3A%28509a75d8455b8f9ffa16bd656ce039d5%29&filter=sc_long_sign&tn=SE_xueshusource_2kduw22v&sc_vurl=http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D2012JCli...25.2609C%26db_key%3DPHY%26link_type%3DABSTRACT&ie=utf-8&sc_us=16784034223311101626
    DeMenocal P. B., 1995: Plio-Pleistocene african climate. Science, 270, 53- 59.10.1126/science.270.5233.5375699515f7e846d-2edb-4a9f-8a90-aab6d05feea75cf8148dba42909b3008a9785940d810http%3A%2F%2Feuropepmc.org%2Fabstract%2FMED%2F7569951refpaperuri:(f4f5b992e7368f454d5cc47f3ce66be2)http://med.wanfangdata.com.cn/Paper/Detail/PeriodicalPaper_PM7569951Marine records of African climate variability document a shift toward more arid conditions after 2.8 million years ago (Ma), evidently resulting from remote forcing by cold North Atlantic sea-surface temperatures associated with the onset of Northern Hemisphere glacial cycles. African climate before 2.8 Ma was regulated by low-latitude insolation forcing of monsoonal climate due to Earth orbital precession. Major steps in the evolution of African hominids and other vertebrates are coincident with shifts to more arid, open conditions near 2.8 Ma, 1.7 Ma, and 1.0 Ma, suggesting that some Pliocene (Plio)-Pleistocene speciation events may have been climatically mediated.
    DeMenocal P. B., 2004: African climate change and faunal evolution during the Pliocene-Pleistocene. Earth and Planetary Science Letters, 220, 3- 24.10.1016/S0012-821X(04)00003-2a446154c591bc1850ec000a2de6f5721http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0012821X04000032http://www.sciencedirect.com/science/article/pii/S0012821X04000032Environmental theories of African faunal evolution state that important evolutionary changes during the Pliocene–Pleistocene interval (the last ca. 5.3 million years) were mediated by changes in African climate or shifts in climate variability. Marine sediment sequences demonstrate that subtropical African climate periodically oscillated between markedly wetter and drier conditions, paced by earth orbital variations, with evidence for step-like (±0.2 Ma) increases in African climate variability and aridity near 2.8 Ma, 1.7 Ma, and 1.0 Ma, coincident with the onset and intensification of high-latitude glacial cycles. Analysis of the best dated and most complete African mammal fossil databases indicates African faunal assemblage and, perhaps, speciation changes during the Pliocene–Pleistocene, suggesting more varied and open habitats at 2.9–2.4 Ma and after 1.8 Ma. These intervals correspond to key junctures in early hominid evolution, including the emergence of our genus Homo . Pliocene–Pleistocene shifts in African climate, vegetation, and faunal assemblages thus appear to be roughly contemporary, although detailed comparisons are hampered by sampling gaps, dating uncertainties, and preservational biases in the fossil record. Further study of possible relations between African faunal and climatic change will benefit from the accelerating pace of important new fossil discoveries, emerging molecular biomarker methods for reconstructing African paleovegetation changes, tephra correlations between terrestrial and marine sequences, as well as continuing collaborations between the paleoclimatic and paleoanthropological communities.
    Dowsett H. J., M. M. Robinson, and K. M. Foley, 2009: Pliocene three-dimensional global ocean temperature reconstruction. Climate of the Past, 5, 769- 783.10.5194/cp-5-769-20095c2cf6266f35801878e7f152c51cb7e8http%3A%2F%2Fwww.oalib.com%2Fpaper%2F1367880http://www.oalib.com/paper/1367880The thermal structure of the mid-Piacenzian ocean is obtained by combining the Pliocene Research, Interpretation and Synoptic Mapping Project (PRISM3) multiproxy sea-surface temperature (SST) reconstruction with bottom water temperature estimates from 27 locations produced using Mg/Ca paleothermometry based upon the ostracod genus Krithe. Deep water temperature estimates are skewed toward the Atlantic Basin (63% of the locations) and represent depths from 1000 m to 4500 m. This reconstruction, meant to serve as a validation data set as well as an initialization for coupled numerical climate models, assumes a Pliocene water mass framework similar to that which exists today, with several important modifications. The area of formation of present day North Atlantic Deep Water (NADW) was expanded and extended further north toward the Arctic Ocean during the mid-Piacenzian relative to today. This, combined with a deeper Greenland-Scotland Ridge, allowed a greater volume of warmer NADW to enter the Atlantic Ocean. In the Southern Ocean, the Polar Front Zone was expanded relative to present day, but shifted closer to the Antarctic continent. This, combined with at least seasonal reduction in sea ice extent, resulted in decreased Antarctic Bottom Water (AABW) production (relative to present day) as well as possible changes in the depth of intermediate waters. The reconstructed mid-Piacenzian three-dimensional ocean was warmer overall than today, and the hypothesized aerial extent of water masses appears to fit the limited stable isotopic data available for this time period.
    Dowsett, H. J., Coauthors, 2010: The PRISM3D paleoenvironmental reconstruction. Stratigraphy, 7, 123- 139.10.1111/j.1475-4983.2010.00949.xec8f197d8418ba1bb2352cd6da5c5834http%3A%2F%2Fwww.researchgate.net%2Fpublication%2F279898329_The_PRISM3D_paleoenvironmental_reconstructionhttp://www.researchgate.net/publication/279898329_The_PRISM3D_paleoenvironmental_reconstructionABSTRACT The Pliocene Research, Interpretation and Synoptic Mapping (PRISM) paleoenvironmental reconstruction is an internally consistent and comprehensive global synthesis of a past interval of relatively warm and stable climate. It is regularly used in model studies that aim to better understand Pliocene climate, to improve model performance in future climate scenarios, and to distinguish model-dependent climate effects. The PRISM reconstruction is constantly evolving in order to incorporate additional geographic sites and environmental parameters, and is continuously refined by independent research findings. The new PRISM three dimensional (3D) reconstruction differs from previous PRISM reconstructions in that it includes a subsurface ocean temperature reconstruction, integrates geochemical sea surface temperature proxies to supplement the faunal-based temperature estimates, and uses numerical models for the first time to augment fossil data. Here we describe the components of PRISM3D and describe new findings specific to the new reconstruction. Highlights of the new PRISM3D reconstruction include removal of Hudson Bay and the Great Lakes and creation of open waterways in locations where the current bedrock elevation is less than 25m above modern sea level, due to the removal of the West Antarctic Ice Sheet and the reduction of the East Antarctic Ice Sheet. The mid-Piacenzian oceans were characterized by a reduced east-west temperature gradient in the equatorial Pacific, but PRISM3D data do not imply permanent El Niño conditions. The reduced equator-to-pole temperature gradient that characterized previous PRISM reconstructions is supported by significant displacement of vegetation belts toward the poles, is extended into the Arctic Ocean, and is confirmed by multiple proxies in PRISM3D. Arctic warmth coupled with increased dryness suggests the formation of warm and salty paleo North Atlantic Deep Water (NADW) and a more vigorous thermohaline circulation system that may have provided the enhanced ocean heat transport necessary to move warm surface water to the Arctic. New deep ocean temperature data also suggests greater warmth and further southward penetration of paleo NADW.
    Dowsett, H. J., Coauthors, 2013: Sea surface temperature of the mid-Piacenzian ocean: a data-model comparison. Scientific Reports,3, doi: 10.1038/srep02013.10.1038/srep02013f07bf1208710c67ffc05d14646aaff2dhttp%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpmc%2Farticles%2FPMC3684808%2Fhttp://www.ncbi.nlm.nih.gov/pmc/articles/PMC3684808/Abstract The mid-Piacenzian climate represents the most geologically recent interval of long-term average warmth relative to the last million years, and shares similarities with the climate projected for the end of the 21(st) century. As such, it represents a natural experiment from which we can gain insight into potential climate change impacts, enabling more informed policy decisions for mitigation and adaptation. Here, we present the first systematic comparison of Pliocene sea surface temperature (SST) between an ensemble of eight climate model simulations produced as part of PlioMIP (Pliocene Model Intercomparison Project) with the PRISM (Pliocene Research, Interpretation and Synoptic Mapping) Project mean annual SST field. Our results highlight key regional and dynamic situations where there is discord between the palaeoenvironmental reconstruction and the climate model simulations. These differences have led to improved strategies for both experimental design and temporal refinement of the palaeoenvironmental reconstruction.
    Haywood A. M., P. J. Valdes, 2004: Modelling Pliocene warmth: Contribution of atmosphere, oceans and cryosphere. Earth and Planetary Science Letters, 218, 363- 377.10.1016/S0012-821X(03)00685-X2fc6377a92b1d50d69bf35f8464057edhttp%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0012821X0300685Xhttp://www.sciencedirect.com/science/article/pii/S0012821X0300685XThe relative role of the atmosphere, oceans and cryosphere in contributing towards middle Pliocene warmth (ca 3 Ma BP) is investigated using the HadCM3 coupled ocean-atmosphere general circulation model. The model was initialised with boundary conditions from the USGS PRISM2 data set and a Pliocene atmospheric CO 2 level of 400 ppmv and run for 300 simulated years. The simulation resulted in a global surface temperature warming of 3 o C compared to present-day. In contrast to earlier modelling experiments for the Pliocene, surface temperatures warmed in most areas including the tropics (1-5 o C). Compared with present-day, the model predicts a general pattern of ocean warming (1-5 o C) in both hemispheres to a depth of 2000 m, below which no significant differences are noted. Sea ice coverage is massively reduced (up to 90%). The flow of the Gulf Stream/North Atlantic Drift is up to 100 mm s -1 greater in the Pliocene case. Analysis of the model-predicted meridional streamfunction suggests a global pattern of reduced outflow of Antarctic bottom water (AABW; up to 5 Sv), a shallower depth for North Atlantic deep water formation and weaker thermohaline circulation (3 Sv). The decrease in AABW occurs mainly in the Pacific rather than Atlantic Ocean. Model diagnostics for heat transports indicate that neither the oceans nor the atmosphere are transporting significantly more heat in the Pliocene scenario. Rather, these results indicate that the major contributing mechanism to global Pliocene warmth was the reduced extent of high-latitude terrestrial ice sheets (50% reduction on Greenland, 33% reduction on Antarctica) and sea ice cover resulting in a strong ice-albedo feedback. These results highlight the need for further studies designed to improve our knowledge regarding Pliocene terrestrial ice configurations.
    Haywood, A. M., Coauthors, 2010: Pliocene model intercomparison project (PlioMIP): Experimental design and boundary conditions (Experiment 1). Geoscientific Model Development, 3, 227- 242.10.5194/gmdd-4-445-2011e171c1be58e3c1281dc1dca40ad5552ehttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F1377401http://www.oalib.com/paper/1377401The Palaeoclimate Modelling Intercomparison Project has expanded to include a model intercomparison for the mid-Pliocene warm period (3.29 to 2.97 million yr ago). This project is referred to as PlioMIP (the Pliocene Model Intercomparison Project). Two experiments have been agreed upon and together compose the initial phase of PlioMIP. The first (Experiment 1) is being performed with atmosphere-only climate models. The second (Experiment 2) utilises fully coupled ocean-atmosphere climate models. Following on from the publication of the experimental design and boundary conditions for Experiment 1 in Geoscientific Model Development, this paper provides the necessary description of differences and/or additions to the experimental design for Experiment 2.
    Haywood A. M., H. J. Dowsett, M. M. Robinson, D. K. Stoll, A. M. Dolan, D. J. Lunt, B. Otto-Bliesner, and M. A. Chandler, 2011: Pliocene model intercomparison project (PlioMIP): Experimental design and boundary conditions (Experiment 2). Geoscientific Model Development, 4, 571- 577.10.5194/gmdd-4-445-2011e171c1be58e3c1281dc1dca40ad5552ehttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F1377401http://www.oalib.com/paper/1377401The Palaeoclimate Modelling Intercomparison Project has expanded to include a model intercomparison for the mid-Pliocene warm period (3.29 to 2.97 million yr ago). This project is referred to as PlioMIP (the Pliocene Model Intercomparison Project). Two experiments have been agreed upon and together compose the initial phase of PlioMIP. The first (Experiment 1) is being performed with atmosphere-only climate models. The second (Experiment 2) utilises fully coupled ocean-atmosphere climate models. Following on from the publication of the experimental design and boundary conditions for Experiment 1 in Geoscientific Model Development, this paper provides the necessary description of differences and/or additions to the experimental design for Experiment 2.
    Haywood, A. M., Coauthors, 2013: Large-scale features of Pliocene climate: results from the Pliocene Model Intercomparison Project. Climate of the Past, 9, 191- 209.10.5194/cp-9-191-2013fa1212961d519728673b6301633100f0http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2980216http://www.oalib.com/paper/2980216Climate and environments of the mid-Pliocene warm period (3.264 to 3.025 Ma) have been extensively studied. Whilst numerical models have shed light on the nature of climate at the time, uncertainties in their predictions have not been systematically examined. The Pliocene Model Intercomparison Project quantifies uncertainties in model outputs through a coordinated multi-model and multi-model/data intercomparison. Whilst commonalities in model outputs for the Pliocene are clearly evident, we show substantial variation in the sensitivity of models to the implementation of Pliocene boundary conditions. Models appear able to reproduce many regional changes in temperature reconstructed from geological proxies. However, data/model comparison highlights that models potentially underestimate polar amplification. To assert this conclusion with greater confidence, limitations in the time-averaged proxy data currently available must be addressed. Furthermore, sensitivity tests exploring the known unknowns in modelling Pliocene climate specifically relevant to the high latitudes are essential (e.g. palaeogeography, gateways, orbital forcing and trace gasses). Estimates of longer-term sensitivity to CO2 (also known as Earth System Sensitivity; ESS), support previous work suggesting that ESS is greater than Climate Sensitivity (CS), and suggest that the ratio of ESS to CS is between 1 and 2, with a "best" estimate of 1.5.
    Haywood, A. M., Coauthors, 2016: The Pliocene Model Intercomparison Project (PlioMIP) Phase 2: Scientific objectives and experimental design. Climate of the Past, 12, 663- 675.10.5194/cp-12-663-2016e67b9378160bee2ffa80ee289b7b597ehttp%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2016CliPa..12..663Hhttp://adsabs.harvard.edu/abs/2016CliPa..12..663HThe Pliocene Model Intercomparison Project (PlioMIP) is a co-ordinated international climate modelling initiative to study and understand climate and environments of the Late Pliocene, as well as their potential relevance in the context of future climate change. PlioMIP examines the consistency of model predictions in simulating Pliocene climate and their ability to reproduce climate signals preserved by geological climate archives. Here we provide a description of the aim and objectives of the next phase of the model intercomparison project (PlioMIP Phase 2), and we present the experimental design and boundary conditions that will be utilized for climate model experiments in Phase 2. Following on from PlioMIP Phase 1, Phase 2 will continue to be a mechanism for sampling structural uncertainty within climate models. However, Phase 1 demonstrated the requirement to better understand boundary condition uncertainties as well as uncertainty in the methodologies used for data-model comparison. Therefore, our strategy for Phase 2 is to utilize state-of-the-art boundary conditions that have emerged over the last 5 years. These include a new palaeogeographic reconstruction, detailing ocean bathymetry and land-ice surface topography. The ice surface topography is built upon the lessons learned from offline ice sheet modelling studies. Land surface cover has been enhanced by recent additions of Pliocene soils and lakes. Atmospheric reconstructions of palaeo-COare emerging on orbital timescales, and these are also incorporated into PlioMIP Phase 2. New records of surface and sea surface temperature change are being produced that will be more temporally consistent with the boundary conditions and forcings used within models. Finally we have designed a suite of prioritized experiments that tackle issues surrounding the basic understanding of the Pliocene and its relevance in the context of future climate change in a discrete way. The Pliocene Model Intercomparison Project (PlioMIP) is a co-ordinated international climate modelling initiative to study and understand climate and environments of the Late Pliocene, as well as their potential relevance in the context of future climate change. PlioMIP examines the consistency of model predictions in simulating Pliocene climate and their ability to reproduce climate signals preserved by geological climate archives. Here we provide a description of the aim and objectives of the next phase of the model intercomparison project (PlioMIP Phase 2), and we present the experimental design and boundary conditions that will be utilized for climate model experiments in Phase 2. Following on from PlioMIP Phase 1, Phase 2 will continue to be a mechanism for sampling structural uncertainty within climate models. However, Phase 1 demonstrated the requirement to better understand boundary condition uncertainties as well as uncertainty in the methodologies used for data-model comparison. Therefore, our strategy for Phase 2 is to utilize state-of-the-art boundary conditions that have emerged over the last 5 years. These include a new palaeogeographic reconstruction, detailing ocean bathymetry and land-ice surface topography. The ice surface topography is built upon the lessons learned from offline ice sheet modelling studies. Land surface cover has been enhanced by recent additions of Pliocene soils and lakes. Atmospheric reconstructions of palaeo-COare emerging on orbital timescales, and these are also incorporated into PlioMIP Phase 2. New records of surface and sea surface temperature change are being produced that will be more temporally consistent with the boundary conditions and forcings used within models. Finally we have designed a suite of prioritized experiments that tackle issues surrounding the basic understanding of the Pliocene and its relevance in the context of future climate change in a discrete way.
    Hill, D. J., Coauthors, 2014: Evaluating the dominant components of warming in Pliocene climate simulations. Climate of the Past, 10, 79- 90.10.5194/cpd-9-1599-20133ddef237ebbf550bca144010fbc7bdcehttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F2980027http://www.oalib.com/paper/2980027The Pliocene Model Intercomparison Project (PlioMIP) is the first coordinated climate model comparison for a warmer palaeoclimate with atmospheric COsignificantly higher than pre-industrial concentrations. The simulations of the mid-Pliocene warm period show global warming of between 1.8 and 3.6 °C above pre-industrial surface air temperatures, with significant polar amplification. Here we perform energy balance calculations on all eight of the coupled ocean-atmosphere simulations within PlioMIP Experiment 2 to evaluate the causes of the increased temperatures and differences between the models. In the tropics simulated warming is dominated by greenhouse gas increases, with the cloud component of planetary albedo enhancing the warming in most of the models, but by widely varying amounts. The responses to mid-Pliocene climate forcing in the Northern Hemisphere midlatitudes are substantially different between the climate models, with the only consistent response being a warming due to increased greenhouse gases. In the high latitudes all the energy balance components become important, but the dominant warming influence comes from the clear sky albedo, only partially offset by the increases in the cooling impact of cloud albedo. This demonstrates the importance of specified ice sheet and high latitude vegetation boundary conditions and simulated sea ice and snow albedo feedbacks. The largest components in the overall uncertainty are associated with clouds in the tropics and polar clear sky albedo, particularly in sea ice regions. These simulations show that albedo feedbacks, particularly those of sea ice and ice sheets, provide the most significant enhancements to high latitude warming in the Pliocene.
    Jiang D. B., H. J. Wang, Z. L. Ding, X. M. Lang, and H. Drange, 2005: Modeling the middle Pliocene climate with a global atmospheric general circulation model. J. Geophys. Res.,110, doi: 10.1029/2004JD005639.10.1029/2004JD0056390ed853686485aea176f6b54b348b27b8http%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1029%2F2004JD005639%2Fabstracthttp://onlinelibrary.wiley.com/doi/10.1029/2004JD005639/abstract[1] A new climate simulation for the middle Pliocene (ca. 3 Ma BP) is performed by a global grid-point atmospheric general circulation model developed at the Institute of Atmospheric Physics (IAP AGCM) with boundary conditions provided by the U. S. Geological Survey's Pliocene Research, Interpretations, and Synoptic Mapping (PRISM) group. It follows that warmer and slightly wetter conditions dominated at the middle Pliocene with a globally annual mean surface temperature increase of 2.60°C, and an increase in precipitation of 4.0% relative to today. At the middle Pliocene, globally annual terrestrial warming was 1.86°C, with stronger warming toward high latitudes. Annual precipitation enhanced notably at high latitudes, with the augment reaching 33.5% (32.5%) of the present value at 60–90°N (60–90°S). On the contrary, drier conditions were registered over most parts at 0–30°N, especially in much of East Asia and the northern tropical Pacific. In addition, both boreal summer and winter monsoon significantly decreased in East Asia at the middle Pliocene. It is indicated that the IAP AGCM simulation is generally consistent with the results from other atmospheric models and agrees well with available paleoclimatic reconstructions in East Asia. Additionally, it is further revealed that the PRISM warmer sea surface temperature and reduced sea ice extent are main factors determining the middle Pliocene climate. The simulated climatic responses arising from the PRISM reconstructed vegetation and continental ice sheet cannot be neglected on a regional scale at mid to high latitudes (like over Greenland and the Qinghai-Tibetan Plateau, and around the circum-Antarctic) but have little influence on global climate.
    Kamae Y., H. Ueda, 2012: Mid-Pliocene global climate simulation with MRI-CGCM2.3: Set-up and initial results of PlioMIP experiments 1 and 2. Geoscientific Model Development, 5, 793- 808.10.5194/gmdd-5-383-2012fc3aacae-ed47-42dc-9326-0c27919ef7b7e23c70c5aae95f6720aadda883b338c0http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2158126refpaperuri:(3c706745b7c63a786d07a32a42b08bcc)http://www.oalib.com/paper/2158126The mid-Pliocene (3.3 to 3.0 million yr ago), a globally warm period before the Quaternary, is recently attracting attention as a new target for paleoclimate modelling and data-model synthesis. This paper reports set-ups and results of experiments proposed in Pliocene Model Intercomparison Project (PlioMIP) using with a global climate model, MRI-CGCM2.3. We conducted pre-industrial and mid-Pliocene runs by using of the coupled atmosphere-ocean general circulation model (AOGCM) and its atmospheric component (AGCM) for the PlioMIP Experiments 2 and 1, respectively. In addition, we conducted two types of integrations in AOGCM simulation, with and without flux adjustments on sea surface. General characteristics of differences in the simulated mid-Pliocene climate relative to the pre-industrial in the three integrations are compared in this study. Generally, difference of simulated surface climate between AGCM and AOGCM is larger than that between the two AOGCM runs, with and without flux adjustments. The simulated climate shows different pattern between AGCM and AOGCM particularly over low latitude oceans, subtropical land regions, and high latitude oceans. The AOGCM simulations do not reproduce wetter environment in the subtropics relative to the present-day, which is suggested by terrestrial proxy data. The differences between the two types of AOGCM runs are little over the land but evident over the ocean particularly in the North Atlantic and polar regions.
    Kamae Y., H. Ueda, and A. Kitoh, 2011: Hadley and walker circulations in the mid-pliocene warm period simulated by an atmospheric general circulation model. J. Meteor. Soc. Japan,89, doi: 10.2151/jmsj.2011-505.10.2151/jmsj.2011-5050f0ea724652f40e14c3e409421767bc2http%3A%2F%2Fci.nii.ac.jp%2Fnaid%2F40019052107http://ci.nii.ac.jp/naid/40019052107The mid-Pliocene warm period (3 million years ago; 3 Ma) is one of the plausible scenarios which provide insight into the climate system in a globally warmer world as projected by climate models for the future. The reconstructed sea surface temperature (SST) by the Pliocene Research, Interpretation and Synoptic Mapping phase 3 (PRISM3) reveals that salient warming occurs in the higher latitudes together with weakening of surface cooling in the equatorial and coastal upwelling regions. The sensitivity of an atmospheric general circulation model (AGCM) is studied by prescribing the surface condition based on the PRISM3 paleoenvironmental reconstructions. The simulated Walker circulation generally slows down, inducing convergent anomaly over the African continent and divergent anomaly over the Asian monsoon region at the lower troposphere; and vice versa at the upper troposphere in response to the reduced east-west gradient of the tropical SST in that period. The ascending branch of the Hadley cell expands poleward, implying a weakening of the meridional circulation in response to the warmer SST in the higher latitudes. To identify the physical reason for the modulation of the wet-dry climatological pattern in low latitudes, additional sensitivity experiments were conducted by changing the configurations of ice-sheet cover, vegetation and zonal patterns of the SST. The results indicate that the reduction of meridional and zonal gradient of tropical SST is the key factor for the expansion of proxy-suggested wetter climate over Africa.
    Kroepelin, S., Coauthors, 2006: Revisiting the age of the Sahara desert. Science, 312, 1138- 1139.10.1126/science.112016116469920982ce8a2-0640-4def-a82c-615efff632e110005b45275bd6263bc8ef31e209b790http%3A%2F%2Feuropepmc.org%2Fabstract%2FMED%2F16469920refpaperuri:(7b32d7a668eb5b8ee863cf6d96dd0e91)http://med.wanfangdata.com.cn/Paper/Detail/PeriodicalPaper_PM16469920In the Sahara region, the age of onset of the desert condition has been uncertain until now. Here we report on the discovery of 7,000,000-year-old eolian dune deposits from the northern Chad Basin. This geological archive is the oldest known evidence for desert occurrence in the Sahara.
    Kutzbach J. E., Z. Liu, 1997: Response of the African monsoon to orbital forcing and ocean feedbacks in the middle holocene. Science, 278, 440- 443.10.1126/science.278.5337.440c3bdec54b3ed46f37d1ca5cbbcebe0c4http%3A%2F%2Fwww.jstor.org%2Fstable%2F2894916http://www.jstor.org/stable/2894916Simulations with a climate model that asynchronously couples the atmosphere and the ocean showed that the increased amplitude of the seasonal cycle of insolation in the Northern Hemisphere 6000 years ago could have increased tropical Atlantic sea surface temperatures in late summer. The simulated increase in sea surface temperature and associated changes in atmospheric circulation enhanced the summer monsoon precipitation of northern Africa by more than 25 percent, compared with the middle Holocene simulation with prescribed modern sea surface temperatures, and provided better agreement with paleorecords of enhanced monsoons.
    Larrasoa\ na , J. C., A. P. Roberts, E. J. Rohling, M. Winklhofer, R. Wehausen, 2003: Three million years of monsoon variability over the northern Sahara. Climate Dyn., 21, 689- 698.10.1007/s00382-003-0355-zafc6648a116aa13d25c5a848405802f8http%3A%2F%2Fwww.springerlink.com%2Fcontent%2Fd1q3956eegky68ym%2Fhttp://www.springerlink.com/content/d1q3956eegky68ym/We present a 3 million year record of aeolian dust supply into the eastern Mediterranean Sea, based on hematite contents derived from magnetic properties of sediments from Ocean Drilling Program Site 967. Our record has an average temporal resolution of ?400 years. Geochemical data validate this record of hematite content as a proxy for the supply of aeolian dust from the Sahara. We deduce that the aeolian hematite in eastern Mediterranean sediments derives from the eastern Algerian, Libyan, and western Egyptian lowlands located north of the central Saharan watershed (?21°N). In corroboration of earlier work, we relate dust flux minima to penetration of the African summer monsoon front to the north of the central Saharan watershed. This would have enhanced soil humidity and vegetation cover in the source regions, in agreement with results from "green Sahara" climate models. Our results indicate that this northward monsoon penetration recurred during insolation maxima throughout the last 3 million years. As would be expected, this orbital precession-scale mechanism is modulated on both short (?100-kyr) and long (?400-kyr) eccentricity time scales. We also observe a strong expression of the ?41-kyr (obliquity) cycle, which we discuss in terms of high- and low-latitude mechanisms that involve Southern Hemisphere meridional temperature contrasts and shifts in the latitudes of the tropics, respectively. We also observe a marked increase in sub-Milankovitch variability around the mid-Pleistocene transition (?0.95 Ma), which suggests a link between millennial-scale climate variability, including monsoon dynamics, and the size of northern hemisphere ice sheets.
    Lawrence, D. M., Coauthors, 2011: Parameterization improvements and functional and structural advances in version 4 of the Community Land Model. Journal of Advances in Modeling Earth Systems,3, doi: 10.1029/2011MS00045.10.1029/2011MS0000456cfd19302af11dfaa7f989baaf0faa9chttp%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1029%2F2011MS00045%2Fcitedbyhttp://onlinelibrary.wiley.com/doi/10.1029/2011MS00045/citedbyThe Community Land Model is the land component of the Community Climate System Model. Here, we describe a broad set of model improvements and additions that have been provided through the CLM development community to create CLM4. The model is extended with a carbon-nitrogen (CN) biogeochemical model that is prognostic with respect to vegetation, litter, and soil carbon and nitrogen states and vegetation phenology. An urban canyon model is added and a transient land cover and land use change (LCLUC) capability, including wood harvest, is introduced, enabling study of historic and future LCLUC on energy, water, momentum, carbon, and nitrogen fluxes. The hydrology scheme is modified with a revised numerical solution of the Richards equation and a revised ground evaporation parameterization that accounts for litter and within-canopy stability. The new snow model incorporates the SNow and Ice Aerosol Radiation model (SNICAR) - which includes aerosol deposition, grain-size dependent snow aging, and vertically-resolved snowpack heating - as well as new snow cover and snow burial fraction parameterizations. The thermal and hydrologic properties of organic soil are accounted for and the ground column is extended to 50-m depth. Several other minor modifications to the land surface types dataset, grass and crop optical properties, surface layer thickness, roughness length and displacement height, and the disposition of snow-capped runoff are also incorporated. The new model exhibits higher snow cover, cooler soil temperatures in organic-rich soils, greater global river discharge, and lower albedos over forests and grasslands, all of which are improvements compared to CLM3.5. When CLM4 is run with CN, the mean biogeophysical simulation is degraded because the vegetation structure is prognostic rather than prescribed, though running in this mode also allows more complex terrestrial interactions with climate and climate change.
    Lebatard, A. E., Coauthors, 2010: Application of the authigenic 10Be/9Be dating method to continental sediments: Reconstruction of the Mio-Pleistocene sedimentary sequence in the early hominid fossiliferous areas of the northern Chad Basin. Earth and Planetary Science Letters, 297, 57- 70.10.1016/j.epsl.2010.06.003ad5c8f87-9056-4b47-b9f4-08b99872494f6d304231800e69bee8936b9eab2a80d1http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0012821X10003778refpaperuri:(2827fb9af751857d9b83eb599f614a64)http://www.sciencedirect.com/science/article/pii/S0012821X10003778The concentrations of atmospheric cosmogenic Be normalized to the solubilized fraction of its stable isotope Be have been measured in the authigenic phase leached from silicated continental sediments deposited since the upper Miocene in the northern Chad Basin. This method is validated by the systematic congruence with the biochronological estimations based on the fossil mammal evolutive degree of faunal assemblages. The fifty-five authigenic Be/ Be ages obtained along 12 logs distributed along two West-East cross sections that encompass best representative Mio-Pliocene outcrops including paleontological sites show a systematic stratigraphic decrease when considering all studied sedimentary facies extending from the Pleistocene up to 8 Ma and allow performing geologic correlations otherwise impossible in the studied area. The resulting global sequence evidences and temporally specifies the succession of the main paleoenvironments that have developed in this region since the Miocene. Under the special conditions encountered in the northern Chad Basin, this study demonstrates that the authigenic Be/ Be ratio may be used as a dating tool of continental sedimentary deposits from 1 to 8 Ma. The half-life of Be theoretically allowing dating up to 14 Ma, it may have fundamental implications on important field research such as paleoclimatology and, through the dating of fossiliferous deposits in paleontology and paleoanthropology.
    Levin N. E., J. Quade, S. W. Simpson, S. Semaw, and M. Rogers, 2004: Isotopic evidence for Plio-Pleistocene environmental change at Gona, Ethiopia. Earth and Planetary Science Letters, 219, 93- 110.10.1016/S0012-821X(03)00707-6d638c704-d302-4f64-ae22-a2aaa3d632ba39a4a68251824cbe284486a51e935fd6http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0012821X03007076refpaperuri:(0abff45bab5921c922081b7a52f8a59f)http://www.sciencedirect.com/science/article/pii/S0012821X03007076A 4.5 Ma record of fluvial and lacustrine deposits is well exposed at Gona, in the Afar Depression of Ethiopia. We use isotopic values of pedogenic carbonate and fossil teeth to reconstruct Plio-Pleistocene environmental change at Gona. An increase in δ C values of pedogenic carbonates since 4.5 Ma points to a shift from woodlands to grassy woodlands in the early Pliocene, -10.4 to -3.9‰ (VPDB), to more open but still mixed environments in the late Pleistocene, -3.0 to -1.4‰ (VPDB). This pattern is also seen in isotopic records elsewhere in East Africa. However, at 1.5 Ma the higher proportion of C grasses at Gona is largely a result of a local facies shift to more water-limited environments. The wide range of δ C values of pedogenic carbonate within single stratigraphic levels indicates a mosaic of vegetation for all time intervals at Gona that depends on depositional environment. Elements of this mosaic are reflected in δ C values of both modern plants and soil organic matter and Plio-Pleistocene soil carbonate, indicating higher amounts of C grasses with greater distance from a river channel in both the modern and ancient Awash River systems. δ O values of pedogenic carbonates increase up-section from -11.9‰ in the early Pliocene to -6.4‰ (VPDB) in the late Pleistocene. The wide range of δ O values in paleovertisol carbonates from all stratigraphic levels probably reflects short-term climate changes and periods of strong evaporation throughout the record. Based on the comparison between δ O values of Plio-Pleistocene pedogenic carbonates and modern waters, we estimate that there has been a 6.5‰ increase in mean annual δ O values of meteoric water since 4.5 Ma. δ O values of pedogenic carbonate from other East African records indicate a similar shift. Increasing aridity and fluctuations in the timing and source of rainfall are likely responsible for the changes in δ O values of East African pedogenic carbonates through the Plio-Pleistocene.
    Levin N. E., F. H. Brown, A. K. Behrensmeyer, R. Bobe, and T. E. Cerling, 2011: Paleosol carbonates from the Omo Group: Isotopic records of local and regional environmental change in East Africa. Palaeogeography, Palaeoclimatology,Palaeoecology, 307, 75- 89.10.1016/j.palaeo.2011.04.026eb02f91709ba1b77b20c979781566f81http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0031018211002288http://www.sciencedirect.com/science/article/pii/S0031018211002288Pliocene and Pleistocene sedimentary rocks from the Omo–Turkana Basin in East Africa are well known for fossil and archeological evidence of human evolution and provide a unique opportunity to study four million years of environmental change in a rift basin. This study uses carbon and oxygen isotope ratios of pedogenic carbonates to examine environmental variability across ~5000km 2 within the Omo–Turkana Basin. An expanded isotopic dataset, including the first isotopic data on pedogenic carbonates from the Shungura Formation and new data from the Nachukui and Koobi Fora formations, is compared to published isotopic records from both the Omo–Turkana Basin and the lower Awash Basin, Ethiopia. Regionally, the carbon isotope record indicates a steady increase of C 4 vegetation in floodplain environments for the past 4million years. The oxygen isotopic record indicates that the isotopic composition of rainfall was depleted in 18 O relative to today's waters and that both basins likely received more rainfall in the Pliocene than today. A shift to higher δ 18 O values in paleosol carbonate after 2Ma in the Omo–Turkana Basin but not in the lower Awash Basin suggests that the ecology and hydrology in these two rift basins were influenced by different climatic regimes. In addition to regional trends, pedogenic carbonates sampled from different parts of the basin show that the distribution of C 4 vegetation and soil water δ 18 O values varied with proximity to the axial river system, and specifically that C 3 vegetation was more dominant in soils of the Shungura Formation compared with coeval sediments downstream in the Nachukui and Koobi Fora formations. This large isotopic dataset from pedogenic carbonates provides the opportunity to examine how terrestrial systems responded to global climate change during the last 4million years, from both local and regional perspectives. The isotopic data indicate that local basin and climate dynamics strongly influenced the impact of large-scale environmental change in East African rift basins.
    Li X. Y., D. B. Jiang, Z. S. Zhang, R. Zhang, Z. P. Tian, and Q. Yan, 2015: Mid-Pliocene Westerlies from PlioMIP Simulations. Adv. Atmos. Sci.,32, 909-923, doi: 10.1007/s00376-014-4171-7.10.1007/s00376-014-4171-7340b51653e5fa274b35c52c4777c99f6http%3A%2F%2Fd.wanfangdata.com.cn%2FPeriodical%2Fdqkxjz-e201507003http://d.wanfangdata.com.cn/Periodical/dqkxjz-e201507003The midlatitude westerlies are one of the major components of the global atmospheric circulation. They play an important role in midlatitude weather and climate, and are particularly significant in interpreting aeolian sediments. In this study, we analyzed the behavior and the possible mechanism involved in the change of the westerlies, mainly in terms of the jet stream position, in the mid-Pliocene warm period(3.3 to 3.0 million years ago) using simulations of 15 climate models from the Pliocene Model Intercomparison Project(Plio MIP). Compared to the reference period, the mid-Pliocene midlatitude westerlies generally shifted poleward(approximately 3.6 of latitude in the Northern Hemisphere and 1.9 of latitude in the Southern Hemisphere at 850 h Pa level) with a dipole pattern. The dipole pattern of the tropospheric zonal wind anomalies was closely related to the change of the tropospheric meridional temperature gradient as a result of thermal structure adjustment.The poleward shift of the midlatitude westerly jet corresponded to the poleward shift of the mean meridional circulation.The sea surface temperatures and sea ice may have affected the simulated temperature structure and zonal winds, causing the spread of the westerly anomalies in the mid-Pliocene between the atmosphere-only and coupled atmosphere cean general circulation model simulations.
    Neale R. B., J. Richter, S. Park, P. H. Lauritzen, S. J. Vavrus, P. J. Rasch, and M. H. Zhang, 2013: The mean climate of the Community Atmosphere Model (CAM4) in forced SST and fully coupled experiments. J.Climate, 26, 5150- 5168.10.1175/JCLI-D-12-00236.1eb23389409ef6dfd676fdf44eef8db00http%3A%2F%2Fwww.researchgate.net%2Fpublication%2F224017886_The_mean_climate_of_the_Community_Atmosphere_Model_%28CAM4%29_in_forced_SST_and_fully_coupled_experimentshttp://www.researchgate.net/publication/224017886_The_mean_climate_of_the_Community_Atmosphere_Model_(CAM4)_in_forced_SST_and_fully_coupled_experimentsAbstract The Community Atmosphere Model, version 4 (CAM4), was released as part of the Community Climate System Model, version 4 (CCSM4). The finite volume (FV) dynamical core is now the default because of its superior transport and conservation properties. Deep convection parameterization changes include a dilute plume calculation of convective available potential energy (CAPE) and the introduction of convective momentum transport (CMT). An additional cloud fraction calculation is now performed following macrophysical state updates to provide improved thermodynamic consistency. A freeze-drying modification is further made to the cloud fraction calculation in very dry environments (e.g., the Arctic), where cloud fraction and cloud water values were often inconsistent in CAM3. In CAM4 the FV dynamical core further degrades the excessive trade-wind simulation, but reduces zonal stress errors at higher latitudes. Plume dilution alleviates much of the midtropospheric tropical dry biases and reduces the persistent monsoon precipitation biases over the Arabian Peninsula and the southern Indian Ocean. CMT reduces much of the excessive trade-wind biases in eastern ocean basins. CAM4 shows a global reduction in cloud fraction compared to CAM3, primarily as a result of the freeze-drying and improved cloud fraction equilibrium modifications. Regional climate feature improvements include the propagation of stationary waves from the Pacific into midlatitudes and the seasonal frequency of Northern Hemisphere blocking events. A 1° versus 2° horizontal resolution of the FV dynamical core exhibits superior improvements in regional climate features of precipitation and surface stress. Improvements in the fully coupled mean climate between CAM3 and CAM4 are also more substantial than in forced sea surface temperature (SST) simulations.
    Prescott C. L., A. M. Haywood, A. M. Dolan, S. J. Hunter, J. O. Pope, and S. J. Pickering, 2014: Assessing orbitally-forced interglacial climate variability during the mid-Pliocene Warm Period. Earth and Planetary Science Letters, 400, 261- 271.10.1016/j.epsl.2014.05.03088301e5a07a09124614f3fd3c1832668http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS0012821X1400332Xhttp://www.sciencedirect.com/science/article/pii/S0012821X1400332XThe traditional view of the Pliocene is one of an epoch with higher than present global mean annual temperatures (652 to 3 °C) and stable climate conditions. Published data-model comparisons for the mid-Pliocene Warm Period (mPWP: 653.3 to 3 million years ago) have identified specific regions of concordance and discord between climate model outputs and marine/terrestrial proxy data. Due to the time averaged nature of global palaeoenvironmental syntheses, it has been hypothesised that climate variability during interglacial events within the mPWP could contribute to site-specific data/model disagreement. The Hadley Centre Coupled Climate Model Version 3 (HadCM3) is used to assess the nature of climate variability around two interglacial events within the mPWP that have different characteristics of orbital forcing (Marine Isotope Stages KM5c and K1). Model results indicate that ±20 kyr on either side of the MIS KM5c, orbital forcing produced a less than 1 °C change in global mean annual temperatures. Regionally, mean annual surface air temperature (SAT) variability can reach 2 to 3 °C. Seasonal variations exceed those predicted for the annual mean and can locally exceed 5 °C. Simulations 20 kyr on either side of MIS K1 show considerably increased variability in relation to KM5c.
    Rosenbloom N. A., B. L. Otto-Bliesner, E. C. Brady, and P. J. Lawrence, 2013: Simulating the mid-Pliocene warm period with the CCSM4 model. Geoscientific Model Development, 6, 549- 561.10.5194/gmdd-5-4269-20122f158a85d9339c43ac43a09b3070b902http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2156291http://www.oalib.com/paper/2156291This paper describes the experimental design and model results from a 500 yr fully coupled Community Climate System, version 4, simulation of the mid- Pliocene Warm Period (mPWP) (ca. 3.3-3.0 Ma). We simulate the mPWP using the "alternate" protocol prescribed by the Pliocene Model Intercomparison Project (PlioMIP) for the AOGCM simulation (Experiment 2). Results from the CCSM4 mPWP simulation show a 1.9 00°C increase in global mean annual temperature compared to the 1850 preindustrial control, with a polar amplification of ~3 times the global warming. Global precipitation increases slightly by 0.09mmday-1 and the monsoon rainfall is enhanced, particularly in the Northern Hemisphere (NH). Areal sea ice extent decreases in both hemispheres but persists through the summers. The model simulates a relaxation of the zonal sea surface temperature (SST) gradient in the tropical Pacific, with the El Ni01±o-Southern Oscillation (Ni01±o3.4) ~ 20% weaker than the preindustrial and exhibiting extended periods of quiescence of up to 150 yr. The maximum Atlantic meridional overturning circulation and northward Atlantic oceanic heat transport are indistinguishable from the control. As compared to PRISM3, CCSM4 overestimates Southern Hemisphere (SH) sea surface temperatures, but underestimates NH warming, particularly in the North Atlantic, suggesting that an increase in northward ocean heat transport would bring CCSM4 SSTs into better alignment with proxy data.
    Salzmann U., A. M. Haywood, D. J. Lunt, P. J. Valdes, and D. J. Hill, 2008: A new global biome reconstruction and data-model comparison for the middle Pliocene. Global Ecology and Biogeography, 17, 432- 447.10.1111/j.1466-8238.2008.00381.x31dcb70a64209a37fbc06e793762e48chttp%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1111%2Fj.1466-8238.2008.00381.x%2Fcitedbyhttp://med.wanfangdata.com.cn/Paper/Detail?id=PeriodicalPaper_JJ0210375444ABSTRACT Aim68 To produce a robust, comprehensive global biome reconstruction for the Middle Pliocene (3.6–2.602Ma), which is based on an internally consistent palaeobotanical data set and a state-of-the-art coupled climate–vegetation model. The reconstruction gives a more rigorous picture of climate and environmental change during the Middle Pliocene and provides a new boundary condition for future general circulation model (GCM) studies. Location68 Global. Methods68 Compilation of Middle Pliocene vegetation data from 202 marine and terrestrial sites into the comprehensive GIS data base TEVIS (Tertiary Environmental Information System). Translation into an internally consistent classification scheme using 28 biomes. Comparison and synthesis of vegetation reconstruction from palaeodata with the outputs of the mechanistically based BIOME4 model forced by climatology derived from the HadAM3 GCM. Results68 The model results compare favourably with available palaeodata and highlight the importance of employing vegetation–climate feedbacks and the anomaly method in biome models. Both the vegetation reconstruction from palaeobotanical data and the BIOME4 prediction indicate a general warmer and moister climate for the Middle Pliocene. Evergreen taiga as well as temperate forest and grassland shifted northward, resulting in much reduced tundra vegetation. Warm-temperate forests (with subtropical taxa) spread in mid and eastern Europe and tropical savannas and woodland expanded in Africa and Australia at the expense of deserts. Discrepancies which occurred between data reconstruction and model simulation can be related to: (1) poor spatial model resolution and data coverage; (2) uncertainties in delimiting biomes using climate parameters; or (3) uncertainties in model physics and/or geological boundary conditions. Main conclusions68 The new global biome reconstruction combines vegetation reconstruction from palaeobotanical proxies with model simulations. It is an important contribution to the further understanding of climate and vegetation changes during the Middle Pliocene warm interval and will enhance our knowledge about how vegetation may change in the future.
    Salzmann, U., Coauthors, 2013: Challenges in quantifying Pliocene terrestrial warming revealed by data-model discord. Nature Climate Change, 3, 969- 974.10.1038/NCLIMATE200830809ba0858960104b8ae6a47d445711http%3A%2F%2Fwww.nature.com%2Fnclimate%2Fjournal%2Fvaop%2Fncurrent%2Ffull%2Fnclimate2008.htmlhttp://www.nature.com/nclimate/journal/vaop/ncurrent/full/nclimate2008.htmlABSTRACT Comparing simulations of key warm periods in Earth history with contemporaneous geological proxy data is a useful approach for evaluating the ability of climate models to simulate warm, high-CO 2 climates that are unprecedented in the more recent past 1–3 . Here we use a global data set of confidence-assessed, proxy-based temperature estimates and biome reconstructions to assess the ability of eight models to simulate warm terrestrial climates of the Pliocene epoch. The Late Pliocene, 3.6–2.6 million years ago, is an accessi-ble geological interval to understand climate processes of a warmer world 4 . We show that model-predicted surface air temperatures reveal a substantial cold bias in the Northern Hemisphere. Particularly strong data–model mismatches in mean annual temperatures (up to 18 61 C) exist in northern Rus-sia. Our model sensitivity tests identify insufficient temporal constraints hampering the accurate configuration of model boundary conditions as an important factor impacting on data– model discrepancies. We conclude that to allow a more robust evaluation of the ability of present climate models to predict warm climates, future Pliocene data–model comparison studies should focus on orbitally defined time slices 5 . Our understanding of the causes and consequences of global warming relies heavily on climate model simulations conducted under a variety of greenhouse gas emission scenarios 6 . Existing data–model comparisons (DMCs) demonstrate that climate models are generally able to reproduce past warm climates of the past 65 million years (Myr; refs 1–3). However, a common data– model mismatch in high-latitude temperature estimates suggests that many models seem to underestimate polar amplification 3,7 . This has led to an ongoing controversy about the accuracy of DMC studies, which might have been biased by uncertainties in estimating temperatures from geological proxies. Recently published proxy-based temperature reconstructions, suggesting tropical-like climates at southern high latitudes about 53 Myr ago 8 (Ma), have intensified the ongoing debate and highlight the
    Schuster, M., Coauthors, 2009: Chad basin: Paleoenvironments of the Sahara since the Late Miocene. Comptes Rendus Geoscience, 341, 603- 611.10.1016/j.crte.2009.04.00192377b99de538767040f9e7f0ad2f3cahttp%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS1631071309000807http://www.sciencedirect.com/science/article/pii/S1631071309000807Since the mid 1990s, the (MPFT) conducts yearly paleontological field investigations of the Miocene-Pliocene of the Chad Basin. This article synthesizes some of the results of the MPFT, with focus on the Chad Basin development during the Neogene. We propose an overview of the depositional paleoenvironments of this part of Africa at different scales of time and space, based on a multidisciplinary approach (sedimentary geology, geomorphology, geophysic, numerical simulations and geochronology). The Miocene-Pliocene paleoenvironments are examined through the sedimentary archives of the early hominids levels and the Holocene Lake Mega-Chad episode illustrates the last major paleoenvironmental change in this area. The sedimentary record of the Chad Basin since the Late Miocene can be schematized as the result of recurrent interactions from lake to desert environments.
    Sepulchre P., G. Ramstein, F. Fluteau, M. Schuster, J.-J. Tiercelin, and M. Brunet, 2006: Tectonic uplift and Eastern Africa aridification. Science, 313, 1419- 1423.10.1126/science.112915816960002c160306c7c13bc9757becf477bb94893http%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpubmed%2F16960002http://med.wanfangdata.com.cn/Paper/Detail/PeriodicalPaper_PM16960002The history of Eastern African hominids has been linked to a progressive increase of open grassland during the past 8 million years. This trend was explained by global climatic processes, which do not account for the massive uplift of eastern African topography that occurred during this period. Atmosphere and biosphere simulations quantify the role played by these tectonic events. The reduced topographic barrier before 8 million years ago permitted a zonal with associated moisture and strong precipitation. Our results suggest that the uplift itself led to a drastic reorganization of atmospheric , engendering the strong aridification and paleoenvironmental changes suggested by the data.
    Shields C. A., D. A. Bailey, G. Danabasoglu, M. Jochum, J. T. Kiehl, S. Levis, and S. Park, 2012: The low-resolution CCSM4. J.Climate, 25, 3993- 4014.a8d75e3e-e618-4194-9547-5de3b3ea78e0f097e8ed99e3cce25bc5323050e289b5http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D2012JCli...25.3993S%26db_key%3DPHY%26link_type%3DABSTRACTrefpaperuri:(84f50795b6ec9c4f94f6250553707fa2)http://xueshu.baidu.com/s?wd=paperuri%3A%2884f50795b6ec9c4f94f6250553707fa2%29&filter=sc_long_sign&tn=SE_xueshusource_2kduw22v&sc_vurl=http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D2012JCli...25.3993S%26db_key%3DPHY%26link_type%3DABSTRACT&ie=utf-8&sc_us=5240920566939011426
    Sloan L. C., T. J. Crowley, and D. Pollard, 1996: Modeling of middle Pliocene climate with the NCAR GENESIS general circulation model. Marine Micropaleontology, 27, 51- 61.10.1016/0377-8398(95)00063-1a34b45801ed55aa4e09c0867684a127fhttp%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2F0377839895000631http://www.sciencedirect.com/science/article/pii/0377839895000631A climate modeling study was carried out which used boundary conditions created by the USGS PRISM group. The model used for this study is the National Center for Atmospheric Research (NCAR) GENESIS climate model. GENESIS is an atmospheric general circulation model (GCM) that is coupled to a land-surface model and contains submodels (for snow and soil. Boundary conditions incorporated into the model which were specific to the middle Pliocene (~ 3 Ma) are (1) present day continent configuration, modified by a 35 m rise in sea level, (2) modified present day elevations, (3) reduced continental ice cover on both Greenland and Antarctica, (4) Pliocene vegetation, and (5) Pliocene sea surface temperatures (SSTs) and sea ice distribution. Atmospheric pCO 2 and orbital parameters were set at current values. The greatest influence of the specified warm SSTs upon the resulting climate was occurrence of warmer and more humid high latitudes than observed in the current climate, especially in the winter season. The global mean surface temperature was 3.6 °C warmer than in a present day control case, and global mean precipitation increased by 5% relative to the control case, with most excess precipitation occurring over the African continent and the oceans. Zonal winds weakened slightly in the Pliocene case but Hadley cell extent and jet stream locations were unchanged relative to the control case. Model results predict specific areas in which middle Pliocene climate should have differed substantially from the present climate, which can be tested with paleoclimate data.
    Stepanek C., G. Lohmann, 2012: Modelling mid-Pliocene climate with COSMOS. Geoscientific Model Development, 5, 1221- 1243.10.5194/gmdd-5-917-201216091691c45f8969a28e833352faac2ehttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F2158658http://www.oalib.com/paper/2158658In this manuscript we describe the experimental procedure employed at the Alfred Wegener Institute in Germany in the preparation of the simulations for the Pliocene Model Intercomparison Project (PlioMIP). We present a description of the utilized community earth system models (COSMOS) and document the procedures which we applied to transfer the Pliocene Research, Interpretation and Synoptic Mapping Project (PRISM) mid-Pliocene reconstruction into model forcing fields. The model setup and spin-up procedure are described for both the paleo and preindustrial (PI) time-slices of PlioMIP experiments 1 and 2, and general results that depict the performance of our model setup for mid-Pliocene conditions are presented. The mid-Pliocene as simulated with our COSMOS-setup and PRISM boundary conditions is both warmer and wetter than the PI. The globally averaged annual mean surface air temperature in the mid-Pliocene standalone atmosphere (fully coupled atmosphere-ocean) simulation is 17.35 °C (17.82 °C), which implies a warming of 2.23 °C (3.40 °C) relative to the respective PI control simulation.
    Sun Y., G. Ramstein, C. Contoux, and T. Zhou, 2013: A comparative study of large scale atmospheric circulation in the context of future scenario (RCP4.5) and past warmth (Mid-Pliocene). Climate of the Past, 9, 1613- 1627.10.5194/cp-9-1613-20134cb24bf8-a01e-4102-b302-807ddebf2142WOS:000323412600017eceaf7d1fee5c35d3ccadbaac48f0566http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2980125refpaperuri:(ef3e87c71f5924366a51bc536139c7bc)http://www.oalib.com/paper/2980125The mid-Pliocene warm period (similar to 3.3-3.0 Ma) is often considered as the last sustained warm period with close enough geographic configurations compared to the present one associated with atmospheric CO2 concentration (405 +/- 50 ppm) higher than the modern level. For this reason, this period is often considered as a potential analogue for the future climate warming, with the important advantage that for mid-Pliocene many marine and continental data are available. To investigate this issue, we selected the RCP4.5 scenario, one of the current available future projections, to compare the pattern of tropical atmospheric response with the past warm mid-Pliocene climate.<br/>We use three Atmosphere-Ocean General Circulation Model (AOGCM) simulations (RCP4.5 scenario, midPliocene and present-day simulation) carried out with the IPSL-CM5A model and investigate atmospheric tropical dynamics through Hadley and Walker cell responses to warmer conditions, considering that the analysis can provide some assessment of how these circulations will change in the future. Our results show that there is a damping of the Hadley cell intensity in the northern tropics and an increase in both subtropics. Moreover, northern and southern Hadley cells expand poleward. The response of the Hadley cells is stronger for the RCP4.5 scenario than for the mid-Pliocene, but in very good agreement with the fact that the atmospheric CO2 concentration is higher in the future scenario than in the midPliocene (543 versus 405 ppm). Concerning the response of the Walker cell, we show that despite very large similarities, there are also some differences. Common features to both scenarios are: weakening of the ascending branch, leading to a suppression of the precipitation over the western tropical Pacific. The response of the Walker cell is stronger in the RCP4.5 scenario than in the mid-Pliocene but also depicts some major differences, as an eastward shift of its rising branch in the future scenario compared to the mid-Pliocene.<br/>In this paper, we explain the dynamics of the Hadley and Walker cells, and show that despite a minor discrepancy, the mid-Pliocene is certainly an interesting analogue for future climate changes in tropical areas.
    Wang B., J. Liu, H. J. Kim, P. J. Webster, and S. Y. Yim, 2012: Recent change of the global monsoon precipitation (1979-2008). Climate Dyn., 39, 1123- 1135.10.1007/s00382-011-1266-zcfa32521375d365bd658a459c8453f02http%3A%2F%2Fwww.springerlink.com%2Fcontent%2Fc645781101555413%2Fhttp://www.springerlink.com/content/c645781101555413/The global monsoon (GM) is a defining feature of the annual variation of Earth’s climate system. Quantifying and understanding the present-day monsoon precipitation change are crucial for prediction of its future and reflection of its past. Here we show that regional monsoons are coordinated not only by external solar forcing but also by internal feedback processes such as El Ni09o-Southern Oscillation (ENSO). From one monsoon year (May to the next April) to the next, most continental monsoon regions, separated by vast areas of arid trade winds and deserts, vary in a cohesive manner driven by ENSO. The ENSO has tighter regulation on the northern hemisphere summer monsoon (NHSM) than on the southern hemisphere summer monsoon (SHSM). More notably, the GM precipitation (GMP) has intensified over the past three decades mainly due to the significant upward trend in NHSM. The intensification of the GMP originates primarily from an enhanced east–west thermal contrast in the Pacific Ocean, which is coupled with a rising pressure in the subtropical eastern Pacific and decreasing pressure over the Indo-Pacific warm pool. While this mechanism tends to amplify both the NHSM and SHSM, the stronger (weaker) warming trend in the NH (SH) creates a hemispheric thermal contrast, which favors intensification of the NHSM but weakens the SHSM. The enhanced Pacific zonal thermal contrast is largely a result of natural variability, whilst the enhanced hemispherical thermal contrast is likely due to anthropogenic forcing. We found that the enhanced global summer monsoon not only amplifies the annual cycle of tropical climate but also promotes directly a “wet-gets-wetter” trend pattern and indirectly a “dry-gets-drier” trend pattern through coupling with deserts and trade winds. The mechanisms recognized in this study suggest a way forward for understanding past and future changes of the GM in terms of its driven mechanisms.
    Wynn J. G., 2004: Influence of Plio-Pleistocene aridification on human evolution: evidence from paleosols of the Turkana Basin, Kenya. American Journal of Physical Anthropology, 123, 106- 118.10.1002/ajpa.10317147306450889feee127e53d9be03b7f1fab40eb1http%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fajpa.10317%2Fabstracthttp://med.wanfangdata.com.cn/Paper/Detail/PeriodicalPaper_PM14730645Abstract New stable carbon isotope measurements, coupled with paleoprecipitation estimates, both from Plio-Pleistocene paleosols of the Turkana Basin, Kenya, provide a high-resolution record of aridification and increasing C 4 biomass during the past 4.3 Ma. This aridification trend is marked by several punctuations at 3.58–3.35, 2.52–2, and 1.81–1.58 Ma, during which the running mean and variance of δ 13 C and paleoaridity estimates increase, suggesting that the proportion of C 4 biomass increases in savanna mosaics during periods of heightened aridity. Increase in C 4 biomass during these aridification events not only increases the proportion of open habitats, but increases the spatial neg-entropy, or heterogeneity of the ecosystem. The aridification events identified correspond to intervals of increased turnover, but more importantly, increased diversity of bovids. Although the record of hominins from the Turkana Basin lacks the temporal resolution and diversity of the bovid record, the aridification intervals identified are marked by similar increases in the diversity and turnover of hominins. These results support the hypothesis that hominins evolved in savanna mosaics that changed through time, and suggest that the evolution of bovids and hominins was driven by shifts in climatic instability and habitat variability, both diachronic and synchronic. Am J Phys Anthropol, 2003. 08 2003 Wiley-Liss, Inc.
    Yan Q., Z. S. Zhang, H. J. Wang, Y. Q. Gao, and W. P. Zheng, 2012: Set-up and preliminary results of mid-Pliocene climate simulations with CAM3.1. Geoscientific Model Development, 5, 289- 297.10.5194/gmdd-4-3339-201133a66c6ba411c6f19c34dc1257665431http%3A%2F%2Fwww.oalib.com%2Fpaper%2F1376769http://www.oalib.com/paper/1376769The mid-Pliocene warm period ~3.264 to 3.025 Ma) is a potential analogue for future climate under global warming. In this study, we use an atmospheric general circulation model (AGCM) called CAM3.1 to simulate the mid-Pliocene climate with the PRISM3D boundary conditions. The simulations show that the global annual mean surface air temperature (SAT) increases by 2.0 °C in the mid-Pliocene compared with the pre-industrial temperature. The greatest warming occurs at high latitudes of both hemispheres, with little change in SAT at low latitudes. The equator-to-pole SAT gradient is reduced in the mid-Pliocene simulation. The annual mean precipitation is enhanced by 3.6% of the pre-industrial value. However, the changes in precipitation are greater at low latitudes than at high latitudes.
    Zhang R., X. D. Liu, 2010: The effects of tectonic uplift on the evolution of Asian summer monsoon climate since Pliocene. Chinese Journal of Geophysics, 53, 948- 960.10.1002/cjg2.1565b3c97f0e8e1ace99e9d15f06fc9aa40dhttp%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fcjg2.1565%2Ffullhttp://en.cnki.com.cn/Article_en/CJFDTotal-DQWX201012006.htmAbundant geological climatic records indicate that northern Tibetan Plateau and southern-eastern Africa have uplifted significantly since Pliocene, at the same time, the Asian summer monsoon climate has undergone great changes. The connection between them is a hot scientific topic in the earth science field. In this paper we conduct a modeling study to explore the climatic effects of tectonic uplifts in northern Tibetan Plateau and southern-eastern Africa since Pliocene by using the Community Atmosphere Model (CAM3. 1) of National Center for Atmospheric Research (NCAR). The results show that the intensification of Asian summer monsoon since Pliocene has close but differential relationships with the tectonic uplifts in the two regions during this period. The uplift of northern Tibetan Plateau mainly intensifies the summer monsoon and increases the precipitation over northern East Asia, and has less effect on South Asian summer monsoon. Whereas, the uplift of southern-eastern Africa principally strengthens South Asian summer monsoon but has less influence on northern East Asian summer monsoon.
    Zhang, R., Coauthors, 2013a: Mid-Pliocene East Asian monsoon climate simulated in the PlioMIP. Climate of the Past, 9, 2085- 2099.10.5194/cp-9-2085-201329855408-babe-4df6-8851-ce55b50f9919WOS:000326597800004ca370a7a541f620e6b3fd9bb2a1e628chttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F2980366refpaperuri:(a507cf7c5a3c23cc5a4d56f46befcbc4)http://www.oalib.com/paper/2980366Based on simulations with 15 climate models in the Pliocene Model Intercomparison Project (PlioMIP), the regional climate of East Asia (focusing on China) during the mid-Pliocene is investigated in this study. Compared to the pre-industrial, the multi-model ensemble mean (MMM) of all models shows the East Asian summer winds (EASWs) largely strengthen in monsoon China, and the East Asian winter winds (EAWWs) strengthen in south monsoon China but slightly weaken in north monsoon China in the mid-Pliocene. The MMM of all models also illustrates a warmer and wetter mid-Pliocene climate in China. The simulated weakened mid-Pliocene EAWWs in north monsoon China and intensified EASWs in monsoon China agree well with geological reconstructions. However, there is a large model-model discrepancy in simulating mid-Pliocene EAWW, which should be further addressed in the future work of PlioMIP.
    Zhang Z. S., Q. Yan, 2012: Pre-industrial and mid-Pliocene simulations with NorESM-L: AGCM simulations. Geoscientific Model Development, 5, 1033- 1043.10.5194/gmdd-5-1203-20123ab051239ff60b11ca505a8ddffa19e3http%3A%2F%2Fwww.oalib.com%2Fpaper%2F1378522http://www.oalib.com/paper/1378522In the Pliocene Model Intercomparison Project (PlioMIP), two sets of experiments are suggested. One includes a reference and a mid-Pliocene experiment run with atmosphere general circulation models (AGCM experiments, referred to as Experiments I), the other includes a pre-industrial and a mid-Pliocene experiment run with coupled ocean-atmosphere general circulation models (AOGCM experiments, referred to as Experiments II). In this paper, we describe the AGCM experiments with the atmosphere component in the low-resolution version of the Norwegian Earth System Model (NorESM-L), and also assess the potential uncertainties in analyzing mid-Pliocene climate anomalies that might result from the choice of the sea surface temperature (SST) forcing for the reference experiment (pre-industrial or modern). We carry out a mid-Pliocene experiment, a control experiment forced by the modern SST fields, and a pre-industrial experiment forced by the monthly SST fields from HadISST averaged between 1879 and 1900. Our experiments illustrate that the simulated mid-Pliocene global mean annual surface air temperature (SAT) is 17.1 °C. It is 2.5 °C warmer than the control experiment, but 2.7 °C warmer than the pre-industrial experiment. We find that the uncertainties in analyses of mid-Pliocene climate anomalies are small on a global scale, but still large on a regional scale. On the regional scale, these uncertainties should be noted and assessed in future PlioMIP studies.
    Zhang, Z. S., Coauthors, 2012: Pre-industrial and mid-Pliocene simulations with NorESM-L. Geoscientific Model Development, 5, 523- 533.10.5194/gmdd-5-119-2012d06468ef-b746-4b67-8d96-21fb7f03e5be8b3e269a10560494e2fdc11c35866a33http%3A%2F%2Fwww.oalib.com%2Fpaper%2F2156644refpaperuri:(3f23b0478564706dda9482bda1574173)http://www.oalib.com/paper/2156644The mid-Pliocene period (3.3 to 3.0 Ma) is known as a warm climate with atmospheric greenhouse gas levels similar to the present. As the climate at this time was in equilibrium with the greenhouse forcing, it is a valuable test case to better understand the long term response to high levels of atmospheric greenhouse gases. In this study, we use the low resolution version of the Norwegian Earth System Model (NorESM-L) to simulate the pre-industrial and the mid-Pliocene climate. Comparison of the simulation with observations demonstrates that NorESM-L simulates a realistic pre-industrial climate. The simulated mid-Pliocene global mean surface air temperature is 16.7 °C, which is 3.2 °C warmer than the pre-industrial. The simulated mid-Pliocene global mean sea surface temperature is 19.1 °C, which is 2.0 °C warmer than the pre-industrial. The warming is relatively uniform globally, except for a strong amplification at high latitudes.
    Zhang, Z. S., Coauthors, 2013b: Mid-Pliocene Atlantic meridional overturning circulation not unlike modern. Climate of the Past, 9, 1495- 1504.10.5194/cpd-9-1297-2013edd5459f5eac07a0aa5956f7ba9cdc2bhttp%3A%2F%2Fwww.oalib.com%2Fpaper%2F2979046http://www.oalib.com/paper/2979046In the Pliocene Model Intercomparison Project (PlioMIP), eight state-of-the-art coupled climate models have simulated the mid-Pliocene warm period (mPWP, 3.264 to 3.025 Ma). Here, we compare the Atlantic Meridional Overturning Circulation (AMOC), northward ocean heat transport and ocean stratification simulated with these models. None of the models participating in the PlioMIP simulates a strong mid-Pliocene AMOC as suggested by earlier proxy studies. Rather, there is no consistent increase in AMOC maximum among the PlioMIP models. The only consistent change in AMOC is a shoaling of the overturning cell in the Atlantic, and a reduced influence of North Atlantic Deep Water (NADW) at depth in the basin. Furthermore, the simulated mid-Pliocene Atlantic northward heat transport is similar to the pre-industrial. These simulations demonstrate that the reconstructed high latitude mid-Pliocene warming can not be explained as a direct response to an intensification of AMOC and concomitant increase in northward ocean heat transport by the Atlantic.
    Zhang Z. S., G. Ramstein, M. Schuster, C. Li, C. Contoux, and Q. Yan, 2014: Aridification of the Sahara desert caused by Tethys Sea shrinkage during the Late Miocene. Natrue,513, 401-404, doi: 10.1038/nature13705.10.1038/nature1370525230661625c2626cca907aa8fa50646022dd4d2http%3A%2F%2Fwww.nature.com%2Fnature%2Fjournal%2Fv513%2Fn7518%2Fnature13705%2Fmetricshttp://med.wanfangdata.com.cn/Paper/Detail/PeriodicalPaper_PM25230661It is widely believed that the Sahara desert is no more than 652-3million years (Myr) old, with geological evidence showing a remarkable aridification of north Africa at the onset of the Quaternary ice ages. Before that time, north African aridity was mainly controlled by the African summer monsoon (ASM), which oscillated with Earth's orbital precession cycles. Afterwards, the Northern Hemisphere glaciation added an ice volume forcing on the ASM, which additionally oscillated with glacial-interglacial cycles. These findings led to the idea that the Sahara desert came into existence when the Northern Hemisphere glaciated 652-3Myr ago. The later discovery, however, of aeolian dune deposits 657Myr old suggested a much older age, although this interpretation is hotly challenged and there is no clear mechanism for aridification around this time. Here we use climate model simulations to identify the Tortonian stage (657-11Myr ago) of the Late Miocene epoch as the pivotal period for triggering north African aridity and creating the Sahara desert. Through a set of experiments with the Norwegian Earth System Model and the Community Atmosphere Model, we demonstrate that the African summer monsoon was drastically weakened by the Tethys Sea shrinkage during the Tortonian, allowing arid, desert conditions to expand across north Africa. Not only did the Tethys shrinkage alter the mean climate of the region, it also enhanced the sensitivity of the African monsoon to orbital forcing, which subsequently became the major driver of Sahara extent fluctuations. These important climatic changes probably caused the shifts in Asian and African flora and fauna observed during the same period, with possible links to the emergence of early hominins in north Africa.
    Zheng W., Z. Zhang, L. Chen, and Y. Yu, 2013: The mid-Pliocene climate simulated by FGOALS-g2. Geoscientific Model Development, 6, 1127- 1135.10.5194/gmd-6-1127-2013d7a351b7-16a8-442e-b9eb-d1ba16af5e5aWOS:000323981100014d9727956d170f4d3bcbd1981c1dd484bhttp%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F2013GMDD....6.2403Zrefpaperuri:(1c9becad18541f15ba3a24a1ffb71c7a)http://adsabs.harvard.edu/abs/2013GMDD....6.2403ZWithin the framework of Pliocene Model Intercomparison Project (PlioMIP), the mid-Pliocene warm period (mPWP - 3.264-3.025 Ma BP) climate simulated by the Flexible Global Ocean-Atmosphere-Land System model grid-point version g2 (FGOALS-g2) are analysed in this study. Results show that the model reproduces the large-scale features of the global warming over the land and ocean. The simulated mid-Pliocene global annual mean surface air temperature (SAT) and sea surface temperature (SST) are 4.17 and 2.62 degrees C warmer than the preindustrial simulation, respectively. In particular, the feature of larger warming over mid-high latitudes is well captured. In the simulated warm mid-Pliocene climate, the Atlantic Meridional Overturning Circulation (AMOC) and El Nino-Southern Oscillation (ENSO) become weaker.
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Manuscript received: 19 September 2015
Manuscript revised: 15 April 2016
Manuscript accepted: 16 May 2016
通讯作者: 陈斌, bchen63@163.com
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Strengthened African Summer Monsoon in the Mid-Piacenzian

  • 1. Climate Change Research Center, Chinese Academy of Sciences, Beijing 100029
  • 2. Department of Atmospheric Science, School of Environmental Studies, China University of Geosciences , Wuhan 430074
  • 3. Nansen-Zhu International Research Centre, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029
  • 4. Bjerknes Centre for Climate Research, Uni Research, Bergen 5007, Norway
  • 5. School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026
  • 6. Plateau Atmosphere and Environment Key Laboratory of Sichuan Province, College of Atmospheric Sciences, Chengdu University of Information Technology, Chengdu 610225

Abstract: Using model results from the first phase of the Pliocene Model Intercomparison Project (PlioMIP) and four experiments with CAM4, the intensified African summer monsoon (ASM) in the mid-Piacenzian and corresponding mechanisms are analyzed. The results from PlioMIP show that the ASM intensified and summer precipitation increased in North Africa during the mid-Piacenzian, which can be explained by the increased net energy in the atmospheric column above North Africa. Further experiments with CAM4 indicated that the combined changes in the mid-Piacenzian of atmospheric CO2 concentration and SST, as well as the vegetation change, could have substantially increased the net energy in the atmospheric column over North Africa and further intensified the ASM. The experiments also demonstrated that topography change had a weak effect. Overall, the combined changes of atmospheric CO2 concentration and SST were the most important factor that brought about the intensified ASM in the mid-Piacenzian.

1. Introduction
  • The mid-Piacenzian (3.264-3.025 Ma) was the last geological period in Earth's history when the global average temperature was 1.84°C-3.60°C warmer than the pre-industrial period (Haywood et al., 2013). Also, the atmospheric CO2 concentration and paleogeography were comparable to those of today (Dowsett et al., 2010). To a certain extent, the climate of the mid-Piacenzian is reflective of the warmer climate predicted for Earth's near future (Sun et al., 2013). In this regard, the mid-Piacenzian has long been a focus for climate modelling studies (e.g., Chandler et al., 1994; Sloan et al., 1996; Haywood and Valdes, 2004; Jiang et al., 2005). In particular, following the initiation of phase one of the Pliocene Model Intercomparison Project (PlioMIP), involving standardized designs for its simulations (Haywood et al., 2010, 2011), an increasing number of new findings have been achieved from model-model and model-data comparisons (Haywood et al., 2013; Zhang et al., 2013a; Hill et al., 2014; Li et al., 2015).

    To date, studies based on PlioMIP have focused on the large-scale climate and/or the climate in the northern high latitudes. For example, (Haywood et al., 2013) revealed the large-scale features of the simulated mid-Piacenzian climate and reported that models potentially underestimate the temperature at high latitudes. (Dowsett et al., 2013) presented a systematic comparison of simulated SST with the PRISM3 (Pliocene Research, Interpretation and Synoptic Mapping) data, and found that the model results were in good agreement with estimates of mid-Piacenzian SST in most regions, although the PlioMIP models generally underestimated the warming in the North Atlantic. The remarkable warming in the North Atlantic in the mid-Piacenzian was once explained by a stronger Atlantic Meridional Overturning Circulation (AMOC) and Atlantic enhanced northward heat transport (e.g., Dowsett et al., 2009). However, the models of PlioMIP do not produce a stronger AMOC; plus, they simulate similar Atlantic northward heat transport to the pre-industrial level (Zhang et al., 2013b). (Hill et al., 2014) evaluated the causes of the Pliocene atmospheric warming using energy balance calculations, and found that the specified ice sheet, high-latitude vegetation boundary conditions and sea ice/snow albedo feedbacks played very important roles in the warming at high latitudes.

    In addition to the global or high-latitude climate, the tropical climate has also been investigated in the PlioMIP models. (Brierley, 2015) recently found that the PlioMIP ensemble shows unexpected agreement in reducing variability and shifting to lower frequencies of ENSO. Besides, the simulated mid-Piacenzian Walker circulation generally slows and the Hadley cell widens poleward (Kamae et al., 2011; Sun et al., 2013).

    Despite being an important sub-system of the tropical climate, the (West) Africa monsoon, which influences the lives of the human population in climate-sensitive North Africa, has not yet been investigated in PlioMIP. Today, most of North Africa is occupied by the largest non-polar desert, the Sahara (9 400 000 km2), which started to form around 7-11 Ma (Zhang et al., 2014) and has expanded greatly during the last 2 or 3 Ma (Kroepelin et al., 2006). In the mid-Piacenzian, compared to present, the Sahara shrank due to the expansion of tropical savanna and woodland in North Africa, likely indicative of an intensified Africa summer monsoon (ASM) (Kutzbach and Liu, 1997; Zhang et al., 2014).

    In this study, we analyze PlioMIP simulation results to examine the characteristics of the ASM in the mid-Piacenzian. Furthermore, using CAM4, we highlight the importance of different boundary conditions to the ASM intensity.

    The remainder of the paper is organized as follows: In section 2, we briefly describe the PlioMIP models used and the experimental design of the CAM4 experiments. In section 3, we present the model results, including the PlioMIP-simulated ASM and the contributions to the ASM changes based on the CAM4 simulations. Section 4 presents the discussion, and section 5 summarizes the study's key findings.

2. Models and experimental design
  • This study begins by analyzing atmosphere-only simulations from seven AGCMs, and coupled simulations from nine PlioMIP AOGCMs (Table 1). Each model carried out one pre-industrial control experiment and one mid-Piacenzian experiment. In the mid-Piacenzian experiment, PRISM3 data were used as the boundary conditions, including the modification of orography, land cover, and the increase in atmospheric CO2 concentration (from 280 ppm to 405 ppm) in the AOGCMs, as well as the SST and sea ice in the AGCMs, compared with the pre-industrial experiment (Haywood et al., 2010, 2011). Considering the models use different resolutions, we re-gridded all the model results to the same resolution of 2.5°× 2.5° to carry out the multi-model analysis.

    In addition, four experiments were carried out with CAM4 to investigate the climate sensitivity to boundary conditions (Table 2). The horizontal resolution of F09 [roughly 0.9° (lat) × 1.25° (lon)] was adopted, and there were 26 layers in the vertical direction (Neale et al., 2013). This high resolution of CAM4 is able to simulate the large-scale pattern of the modern ASM reasonably well (Cook et al., 2012; Neale et al., 2013), and shows improvements in simulated precipitation, compared with the low resolution version, because of better resolved topography (Shields et al., 2012). Version 4 of the Community Land Model (CLM4) was also included in the simulations (Lawrence et al., 2011). More information about CAM4 and CLM4 can be found in model validation studies in the literature (Shields et al., 2012; Neale et al., 2013).

    We ran the experiments from the pre-industrial period (PI) and step-by-step replaced the topography, vegetation and the combined changes of atmospheric CO2 concentration and SST with mid-Piacenzian boundary conditions using PRISM3 data (Haywood et al., 2010), in order to address how these boundary conditions affected the climate in North Africa (Fig. 1). Aside from the PI control experiment, topography was changed in experiment PI t, vegetation was changed in experiment PI tv, and finally the atmospheric CO2 concentration and SST were further changed in the mid-Piacenzian experiment (MP). All experiments were integrated for 30 years, and all reached a quasi-equilibrium state within the first 10 years. The climatological means from the last 20 years in each experiment are analyzed here, with a focus on the model results in boreal summer (June, July and August).

    Figure 1.  The difference in (a) topography (units: m), (b) summer surface albedo, (c) summer SST (units: $^\circ$C), and (d) winter SST (units: $^\circ$C) between the experiment MP and PI using CAM4. The region indicated by the red box in (a) was selected for the diagnosis in Table 3.

3. Results
  • In the PlioMIP simulations, the ASM became stronger and brought more precipitation to North Africa during the mid-Piacenzian. The multi-model ensemble mean (MMM) of all the models, with the same weight among models, showed that the summer westerly wind in North Africa became stronger during the mid-Piacenzian relative to the pre-industrial (Fig. 2a). Summer precipitation increased by more than 1 mm d-1 in North Africa, particularly between 10° and 20°N (Fig. 2a). Generally, precipitation change in North Africa comes from two major moisture sources——moisture advection and local recycling (Bosmans et al., 2012), which is measured by the ratio of the difference between the precipitation and evaporation anomaly to the precipitation anomaly: \((\Delta P-\Delta E)/\Delta P\), P and E denote precipitation and evaporation. In the region (10°-20°N, 10°W-40°E), approximately 55% of the regional averaged precipitation increase between the mid-Piacenzian and the pre-industrial was due to moisture advection from the tropical Atlantic, and the remaining part was caused by local recycling. Since the moisture advection in this region derived mainly from the intensified ASM, the increased summer precipitation in North Africa likely derived more from the intensified ASM. Along with the intensified ASM and increased precipitation, both the North African monsoon domain (Wang et al., 2012) and the ITCZ (Braconnot et al., 2007) shifted northward during the mid-Piacenzian (Figs. 2a and 3a).

    The intensified ASM was caused by increased net energy in the atmospheric column above North Africa. The MMM indicated that the net energy above North Africa increased significantly (Fig. 4a) because of the marked increase in net heat flux at the model top. This increase in net energy promoted anomalous low-level atmospheric convergence (Fig. 2a) over North Africa (Chou and Neelin, 2003; Zhang et al., 2014). As a result, moist air flow from the ocean penetrated farther inland, which strengthened the ASM and promoted the summer precipitation increase in North Africa (Fig. 2a).

    Figure 2.  Difference in the MMM for summer 850-hPa wind (vectors; units: m s$^-1$) and precipitation (shaded; units: mm d$^-1$) between the mid-Piacenzian and pre-industrial experiments from PlioMIP simulations: (a) is the MMM for all the models; (b) is the MMM for the AGCMs; and (c) is the MMM for the AOGCMs. Regions with an elevation above 1500 m for winds are left blank. The red (mid-Piacenzian) and blue (pre-industrial) dots show the positions of the climatological mean ITCZ, as defined by Braconnot et al. (2007).

    Figure 3.  Monsoon domain (shaded) for the pre-industrial and mid-Piacenzian experiments from PlioMIP simulations: (a) is the MMM for all the models; (b) is the MMM for the AGCMs; and (c) is the MMM for AOGCMs. The light blue areas indicate the regions identified in both experiments, and the dark blue (orange) areas indicate the regions of expansion (retreat) in the mid-Piacenzian compared to the pre-industrial period. Monsoon domains were calculated according to the definition in Wang et al. (2012), with the summer-minus-winter precipitation exceeding 2.0 mm d$^-1$ and the local summer precipitation exceeding 55% of the annual total precipitation. The summer (winter) here is from May to September (November to March).

    Owing to increased net energy in the atmospheric column above North Africa (Figs. 4b vs. 4c), the AGCMs predicted a much stronger ASM than the AOGCMs (Figs. 2b vs. 2c), with a more northward positioning of the North African monsoon domain and the ITCZ than in the AOGCMs (Figs. 2 and 3). The AGCMs use PRISM3 reconstructions, while the AOGCMs include atmosphere-ocean feedback. Thus, the discrepancy in the model results between the AGCMs and AOGCMs was mainly caused by the difference in the SST. Even so, geological evidence indicates that the climate in mid-Piacenzian was up to 5°C cooler than the Late Quaternary in Hadar, Ethiopia (Bonnefille et al., 2004). This evidence, and other temperature estimates available from the tropics, possibly suggest a large overestimation of the SST and surface air temperature (SAT) in the low latitudes by 1°C-6°C in the AOGCMs (Dowsett et al., 2013; Salzmann et al., 2013). If so, this overestimated SST and SAT in the tropics possibly led to the underestimation of the intensified ASM in the AOGCMs.

    Figure 4.  Difference in the MMM for summer net energy [definition in Chou and Neelin (2003)] in the atmospheric column (units: W m$^-2$) between the mid-Piacenzian and pre-industrial experiments from PlioMIP simulations: (a) is the MMM for all the models; (b) is the MMM for the AGCMs; and (c) is the MMM for the AOGCMs.

  • In order to isolate the roles of mid-Piacenzian boundary conditions in the intensified ASM, high-resolution CAM4 experiments were also used to simulate the climate during the mid-Piacenzian (Table 2). In general, CAM4 simulated the intensified ASM and increased precipitation in North Africa well during the mid-Piacenzian, relative to the pre-industrial, agreeing well with the MMM of the PlioMIP models (Figs. 2 and 5a).

    The CAM4 sensitivity experiments showed that the combined changes of atmospheric CO2 concentration and SST were the most important factor to the intensified ASM during the mid-Piacenzian. These combined changes were largely responsible for promoting the warming in North Africa, which changed the temperature gradient (Fig. 6b) and strengthened the thermal low anomalies in North Africa (not shown). These combined changes further enhanced the onshore flow from the ocean. After the change in atmospheric CO2 concentration and SST in experiment MP compared to experiment PI tv, the summer westerly wind strengthened markedly by 1.57 m s-1, averaged within North Africa (5°-30°N, 10°W-40°E), moisture advection intensified (Table 3), and ultimately, the summer precipitation increased significantly by 1.01 mm d-1, with the ITCZ and the northern limit of the North African monsoon domain also shifting northward in North Africa (Fig. 5b).

    Figure 5.  The simulated summer 850-hPa wind (vectors; units: m s$^-1$) and precipitation (shaded; units: mm d$^-1$) changes between experiments using CAM4. Only changes for precipitation and 850-hPa wind (either zonal or meridional wind) that are significant at the 95% confidence level (Student's $t$-test) are shown. Monsoon domains (contours) and the positions of the climatological mean ITCZ (dots) are also shown. Red contours and dots are shown for experiment (a) MP, (b) MP, (c) PI$_\rm tv$ and (d) PI$_\rm t$. Blue contours and dots are shown for experiment (a) PI, (b) PI$_\rm tv$, (c) PI$_\rm t$ and (d) PI.

    Vegetation change was the second most important factor for the increase in intensity of the simulated ASM. Owing to the improved vegetation in experiment PItv, the summer westerly wind strengthened by 0.62 m s-1 and the summer precipitation increased by 0.74 mm d-1, averaged within North Africa (5°-30°N, 10°W-40°E) (Fig. 5c), when compared to experiment PI t. These increases were considerably larger than the changes caused by topography (PI t minus PI) (Fig. 5d). Moreover, the vegetation change also shifted the ITCZ and the northern limit of the North African monsoon domain northward, while the change caused by topography was weak (Figs. 5c and d). Although the vegetation change decreased the surface albedo (Fig. 1b), due to an increase in cloud cover (Table 3), vegetation change finally caused the SAT in North Africa to decrease (Fig. 6c). By comparison, due to the effects of the temperature lapse rate, increased topography caused the SAT to decrease, and vice versa (Fig. 6d).

    The increased intensity of the ASM caused by the changed boundary conditions can also be explained by the increased net energy in the atmospheric column above North Africa (Fig. 7, Table 3). Such increased net energy promoted ascending motion (Fig. 8) and low-level atmospheric convergence (Fig. 5). The combined changes of atmospheric CO2 concentration and SST increased the net heat flux at the model top considerably (Table 3), which resulted from decreased top upwelling longwave flux due to the increased cloud fraction (Table 3). This increased net top heat flux further increased the net energy over most of North Africa (Fig. 7b). The nature of the Pliocene vegetation, with less desert cover and reduced surface albedo, also increased the net heat flux at the model top (Table 3) and further enhanced the net energy over North Africa, in particular between 15°N and 25°N (Fig. 7c). By comparison, the changed topography generally had a weak effect on the increased net energy over North Africa (Fig. 7d, Table 3).

    Figure 6.  The simulated summer changes of SAT (units: $^\circ$C) between experiments using CAM4. Only changes that are significant at the 95% confidence level (Student's $t$-test) are shown.

    Figure 7.  The simulated summer changes of net energy in the atmospheric column (units: W m$^-2$) between experiments using CAM4. Only changes that are significant at the 95% confidence level (Student's $t$-test) are shown.

    Figure 8.  The simulated summer changes of vertical velocity at 500 hPa (units: 100$^-1$ Pa s$^-1$) between experiments using CAM4. Upward motion is negative and downward motion is positive. Only changes that are significant at the 95% confidence level (Student's $t$-test) are shown.

4. Discussion
  • Geological evidence indicates the existence of a wetter environment in North Africa in the mid-Piacenzian. For example, palynological data demonstrate that the desert zone was smaller than today during the mid-Piacenzian (Salzmann et al., 2008), with a much larger tree cover density in both West and East Africa compared to the Late Quaternary (Bonnefille, 2010). Moreover, high δ18O values in soil carbonate and paleoprecipitation estimates also indicate East Africa likely received more rainfall in the mid-Piacenzian (Levin et al., 2004, 2011; Wynn, 2004). Under these wetter conditions, low dust fluxes were present in the Atlantic (e.g., ODP site 664), Arabian Sea (e.g., ODP site 721) and Mediterranean (e.g., ODP site 967) in the mid-Piacenzian (DeMenocal, 1995, 2004; Larrasoa\ na et al., 2003), and the northern Chad Basin in North Africa features lacustrine sediment occurring from 7 to 3 Ma (Schuster et al., 2009; Lebatard et al., 2010).

    The simulated wetter climate in the mid-Piacenzian qualitatively agrees with the geological evidence mentioned above. As shown in the simulation results, the combined changes of atmospheric CO2 concentration and SST, as well as the vegetation change, both contributed more to the increased precipitation, compared with the topography change. Therein, the combined changes of atmospheric CO2 concentration and SST were able to markedly intensify the moisture advection, while the vegetation change intensified more the local recycling in North Africa (Table 3). Since the combined changes of atmospheric CO2 concentration and SST were so important for the increased precipitation during the mid-Piacenzian (Table 3), the moisture advection, mainly from the intensified ASM contributed more, compared with the local recycling, to the increased precipitation in North Africa in the mid-Piacenzian.

    The changes in boundary conditions determine the corresponding climate effects, and the potential uncertainty in boundary conditions may influence the simulated ASM. For example, geological evidence indicates major uplift activity existed in African mountains during the mid to late Pliocene (Sepulchre et al., 2006; Zhang and Liu, 2010). If so, the changed topography perhaps had different climate effects. Moreover, there were also discrepancies in the simulated ASM between the AOGCMs and AGCMs, due to the different SST used. Thus, more studies are needed to reduce the uncertainty in boundary conditions and further check the potential climate effects.

    In addition, more research effort is needed to help understand the orbital-forced changes in precipitation in North Africa within the mid-Piacenzian. The present study focused on the mean climate in the mid-Piacenzian. Orbital-forced climate changes, including precipitation in North Africa, during interglacial events within the mid-Piacenzian, could have been substantial (Prescott et al., 2014). The second phase of PlioMIP will focus on the identification of a "time slice" (MIS KM5c; 3.205 Ma) that has similar orbital forcing to today (Haywood et al., 2016). Even so, studies on orbital-forced changes of precipitation in North Africa during interglacial events are still needed, to better understand the ASM within the mid-Piacenzian, as well as the model-data discord.

5. Summary
  • In the MMM result of all models from PlioMIP, the ASM strengthened and the precipitation increased over North Africa in the mid-Piacenzian, compared to the pre-industrial. The strengthened monsoon activity was caused by the increased net energy in the atmospheric column over North Africa. Furthermore, CAM4 simulations indicated that the combined changes of atmospheric CO2 concentration and SST, as well as the vegetation change, were able to increase the net energy in the atmospheric column over North Africa, which promoted the strengthened ASM and increased the precipitation in the region.

Reference

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