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Barotropic Processes Associated with the Development of the Mei-yu Precipitation System


doi: 10.1007/s00376-015-5146-z

  • The barotropic processes associated with the development of a precipitation system are investigated through analysis of cloud-resolving model simulations of Mei-yu torrential rainfall events over eastern China in mid-June 2011. During the model integration period, there were three major heavy rainfall events: 9-12, 13-16 and 16-20 June. The kinetic energy is converted from perturbation to mean circulations in the first and second period, whereas it is converted from mean to perturbation circulations in the third period. Further analysis shows that kinetic energy conversion is determined by vertical transport of zonal momentum. Thus, the prognostic equation of vertical transport of zonal momentum is derived, in which its tendency is associated with dynamic, pressure gradient and buoyancy processes. The kinetic energy conversion from perturbation to mean circulations in the first period is mainly associated with the dynamic processes. The kinetic energy conversion from mean to perturbation circulations in the third period is generally related to the pressure gradient processes.
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    Li X. F., S. T. Gao, 2012: Precipitation Modeling and Quantitative Analysis. Springer,Dordrecht, 240 pp.10.1007/978-94-007-2381-887b7dbf8-dfc6-42c2-a0a7-c8eabe16eb80e5bf40ca3f1c52c208260310236b78bchttp%3A%2F%2Flink.springer.com%2F978-94-007-2381-8refpaperuri:(e325017cdff17cac5f7d04bd3472e326)http://link.springer.com/978-94-007-2381-8The book examines surface rainfall processes through cloud-resolving modeling and quantitative analysis of surface rainfall budget and summarizes modeling and analysis results in recent seven years. The book shows validation of precipitation modeling against observations and derives a set of diagnostic precipitation equations. The book provides detailed discussions of the applications of precipitation equations to the examination of effects of sea surface temperature, vertical wind shear, radiation, and ice clouds on torrential rainfall processes in the tropics and mid-latitudes, and to the studies of sensitivity of precipitation modeling to uncertainty of the initial conditions and to the estimate of precipitation efficiency. The book can be used as a text book for graduate students and will be beneficial to researchers and forecasters for precipitation process studies and operational forecasts.Xiaofan Li is a physical scientist at the Center for Satellite Applications and Research, National Environmental Satellite, Data, and Information Service, National Oceanic and Atmospheric Administration, Camp Springs, Maryland, USA. He has a doctorate in meteorology from the University of Hawaii at Manoa, Honolulu, USA and a master s degree in meteorology from Nanjing University of Information Science and Technology, Nanjing, China.Shouting Gao is a professor at the Laboratory of Cloud-Precipitation Physics and Severe Storm, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing, China. He has a doctorate and a master s degree in meteorology from the Institute of Atmospheric Physics, Beijing, China.
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    Lin Y.-L., R. D. Farley, and H. D. Orville, 1983: Bulk parameterization of the snow field in a cloud model. J. Climate Appl. Meteor., 22, 1065- 1092.10.1175/1520-0450(1983)0222.0.CO;29190891c3775ec6ca868fe681504eba0http%3A%2F%2Fci.nii.ac.jp%2Fnaid%2F10013127356%2Fhttp://ci.nii.ac.jp/naid/10013127356/Abstract A two-dimensional, time-dependent cloud model has been used to simulate a moderate intensity thunderstorm for the High Plains region. Six forms of water substance (water vapor, cloud water, cloud ice, rain, snow and hail, i.e., graupel) are simulated. The model utilizes the -渂ulk water- microphysical parameterization technique to represent the precipitation fields which are all assumed to follow exponential size distribution functions. Autoconversion concepts are used to parameterize the collision-coalescence and collision-aggregation processes. Accretion processes involving the various forms of liquid and solid hydrometeors are simulated in this model. The transformation of cloud ice to snow through autoconversion (aggregation) and Bergeron process and subsequent accretional growth or aggregation to form hail are simulated. Hail is also produced by various contact mechanisms and via probabilistic freezing of raindrops. Evaporation (sublimation) is considered for all precipitation particles outside the cloud. The melting of hail and snow are included in the model. Wet and dry growth of hail and shedding of rain from hail are simulated. The simulations show that the inclusion of snow has improved the realism of the results compared to a model without snow. The formation of virga from cloud anvils is now modeled. Addition of the snow field has resulted in the inclusion of more diverse and physically sound mechanisms for initiating the hail field, yielding greater potential for distinguishing dominant embryo types characteristically different from warm- and cold-based clouds.
    Pastushkov R. S., 1975: The effects of vertical wind shear on the evolution of convective clouds. Quart. J. Roy. Meteor. Soc., 101, 281- 291.10.1002/qj.49710142811a8234823c43b75e14680f152335327eehttp%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fqj.49710142811%2Fabstracthttp://onlinelibrary.wiley.com/doi/10.1002/qj.49710142811/abstractAbstract The effects of ambient wind shear U o on the evolution of an isolated three-dimensional convective cloud are studied. Sixteen cases are considered which differ from one another both in the value of U ′ 0 in the initial value of the energy of atmospheric instability per unit height of the unstable layer, E 0 . It is found that convective clouds may be grouped into two types, ‘weak’ and ‘strong’: if E 0 / H < 06165 × 10 2 cm s 612 then convection is ‘weak’; if E 0 06165 × 10 612 cm s 612 then convection is ‘strong’. For ‘weak’ convective clouds there is a critical value of shear, U ′ 0cr | U ′ 0 | < U ′ 0cr there is an inhibiting effect on the development of convection; and for | U ′ 0 | U ′ 0 its evolution is completely suppressed. The essential new result is that ‘strong’ convective clouds are intensified under the effect of U ′ 0 . In this case there is a resonance value of shear, U ′ 0res at which the degree of the intensification of convection has a maximum (30–40%).
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    Rutledge S. A., P. V. Hobbs, 1984: The mesoscale and microscale structure and organization of clouds and precipitation in midlatitude cyclones. XII: A diagnostic modeling study of precipitation development in narrow cold-frontal rainbands. J. Atmos. Sci., 41, 2949- 2972.456879270fd5329b8dc7d947fab97e69http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D1984JAtS...41.2949R%26db_key%3DPHY%26link_type%3DABSTRACT/s?wd=paperuri%3A%28bafd052a30102d877b807965b2be62b9%29&filter=sc_long_sign&tn=SE_xueshusource_2kduw22v&sc_vurl=http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D1984JAtS...41.2949R%26db_key%3DPHY%26link_type%3DABSTRACT&ie=utf-8
    Shen X. Y., Y. Wang, and X. F. Li, 2011: Effects of vertical wind shear and cloud radiative processes on responses of rainfall to the large-scale forcing during pre-summer heavy rainfall over southern China. Quart. J. Roy. Meteor. Soc., 137, 236- 249.10.1002/qj.735b538b8c2-33a7-4c32-a291-ffc9ca02d1cd626136d7a885d5037b4b3d383f4c0426http%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fqj.735%2Fpdfrefpaperuri:(ff92848d2aef39967190127909dfca3a)http://onlinelibrary.wiley.com/doi/10.1002/qj.735/pdfABSTRACT The pre-summer heavy rainfall over southern China during 3-8 June 2008 is simulated using a two-dimensional cloud-resolving model. The model is integrated with imposed zonally uniform vertical velocity, zonal wind, horizontal temperature and vapour advection from National Centers for Environmental Prediction (NCEP)/Global Data Assimilation System (GDAS) data. The effects of vertical wind shear and cloud radiative processes on the response of rainfall to large-scale forcing are analysed through the comparison of two sensitivity experiments with the control experiment. One sensitivity experiment excludes the large-scale vertical wind shear and the other excludes the cloud radiative effects. During the decay phase of convection, the increase in model domain-mean surface rain-rate resulting from the exclusion of vertical wind shear is associated with the slowdown in the decrease of perturbation kinetic energy due to the exclusion of barotropic conversion from mean kinetic energy to perturbation kinetic energy. The increase in domain-mean rain-rate from the exclusion of cloud radiative effects is related to the enhancement of condensation and associated latent heat as a result of strengthened radiative cooling. The increase in the domain-mean surface rain-rate is mainly associated with the increase of convective rainfall, which is in turn related to the local atmospheric change from moistening to drying. During the onset and mature phases of convection, the domain-mean surface rain-rates are generally insensitive to vertical wind shear and cloud radiative effects whereas convective and stratiform rain-rates are sensitive to vertical wind shear and cloud radiative effects. The decrease in convective rain-rate and the increase in stratiform rain-rate are primarily associated with the enhanced transport of hydrometeor concentration from convective regions to raining stratiform regions. Copyright 漏 2011 Royal Meteorological Society
    Soong S.-T., Y. Ogura, 1980: Response of tradewind cumuli to large-scale processes. J. Atmos. Sci., 37, 2035- 2050.10.1175/1520-0469(1980)037<2035:ROTCTL>2.0.CO;2ff29183f-0c94-40ab-a743-344ed26775f0b7378c22aa84e357b292f1c0c7b03256http://www.researchgate.net/publication/234192515_Response_of_Tradewind_Cumuli_to_Large-Scale_Processeshttp://www.researchgate.net/publication/234192515_Response_of_Tradewind_Cumuli_to_Large-Scale_ProcessesABSTRACT The 2-dimensional slab-symmetric numerical cloud model for studying the evolution of an isolated cumulus cloud is extended to investigate the statistical properties of cumulus clouds which would be generated under a given large-scale forcing composed of the horizontal advection of temperature and water vapor mixing ratio, vertical velocity, sea surface temperature and radiative cooling. The model is applied to a case of suppressed weather conditions during BOMEX for the period 22-23 June 1969 when a nearly steady state prevailed. -from Authors
    Soong S.-T., W.-K. Tao, 1980: Response of deep tropical cumulus clouds to mesoscale processes. J. Atmos. Sci., 37, 2016- 2034.9cb2afe5e74b2575cdebc09c8082d7bfhttp%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D1980JAtS...37.2016S%26db_key%3DPHY%26link_type%3DABSTRACT/s?wd=paperuri%3A%280bd9ba2116c04e1b0401e5e152555845%29&filter=sc_long_sign&tn=SE_xueshusource_2kduw22v&sc_vurl=http%3A%2F%2Fadsabs.harvard.edu%2Fcgi-bin%2Fnph-data_query%3Fbibcode%3D1980JAtS...37.2016S%26db_key%3DPHY%26link_type%3DABSTRACT&ie=utf-8
    Sui C. H., K. M. Lau, W. K. Tao, and J. Simpson, 1994: The tropical water and energy cycles in a cumulus ensemble model. Part I: equilibrium climate. J. Atmos. Sci., 51, 711- 728.10.1175/1520-0469(1994)051<0711:TTWAEC>2.0.CO;29f796b7d91f49f15c2596dd8f4a3020chttp%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F1994JAtS...51..711Shttp://adsabs.harvard.edu/abs/1994JAtS...51..711SAbstract A cumulus ensemble model is used to study the tropical water and energy cycles and their role in the climate system. The model includes cloud dynamics, radiative processes, and microphysics that incorporate all important production and conversion processes among water vapor and five species of hydrometeors. Radiative transfer in clouds is parameterized based on cloud contents and size distributions of each bulk hydrometeor. Several model integrations have been carried out under a variety of imposed boundary and large-scale conditions. In Part I of this paper, the primary focus is on the water and heat budgets of the control experiment, which is designed to simulate the convective-搑adiative equilibrium response of the model to an imposed vertical velocity and a fixed sea surface temperature at 28C. The simulated atmosphere is conditionally unstable below the freezing level and close to neutral above the freezing level. The equilibrium water budget shows that the total moisture source, M s , which is contributed by surface evaporation (0.24 M s ) and the large-scale advection (0.76 M s ), all converts to mean surface precipitation P s . Most of M s is transported vertically in convective regions where much of the condensate is generated and falls to surface (0.68 P s ). The remaining condensate detrains at a rate of 0.48 P s and constitutes 65% of the source for stratiform clouds above the melting level. The upper-level stratiform cloud dissipates into clear environment at a rate of 0.14 P s , which is a significant moisture source comparable to the detrained water vapor (0.15 P s ) to the upper troposphere from convective clouds. In the lower troposphere, stratiform clouds evaporate at a rate of 0.41 P s , which is a more dominant moisture source than surface evaporation (0.22 P s ). The precipitation falling to the surface in the stratiform region is about 0.32 P s . The associated latent heating in the water cycle is the dominant source in the heat budget that generates a net upward motion in convective regions, upper stratiform regions (above the freezing level), and a downward motion in the lower stratiform regions. The budgets reveal a cycle of water and energy resulted from radiation-揹ynamic-揷onvection interactions that maintain the equilibrium of the atmosphere.
    Sui C.-H., X. Li, and K.-M. Lau, 1998: Radiative-convective processes in simulated diurnal variations of tropical Oceanic convection. J. Atmos. Sci., 55, 2345- 2357.10.1175/1520-0469(1998)055<2345:RCPISD>2.0.CO;2184a7427-712a-4928-b165-1f3ed1902f43a5659bebf87700e06fd5f4843658e1echttp://www.researchgate.net/publication/249609844_RadiativeConvective_Processes_in_Simulated_Diurnal_Variations_ofTropical_Oceanic_Convectionhttp://www.researchgate.net/publication/249609844_RadiativeConvective_Processes_in_Simulated_Diurnal_Variations_ofTropical_Oceanic_ConvectionPresents an analysis of the diurnal variation of tropical oceanic convection and its association with the energy cycle as simulated by an anelastic cumulus ensemble model. Observations of studies conducted on diurnal variations; Reference to the application of the cumulus ensemble model; Information on the diurnal variations of convection.
    Tao W.-K., J. Simpson, 1993: The Goddard cumulus ensemble model. Part I: model description. Terrestrial Atmospheric and Oceanic Sciences, 4, 35- 72.8e5bceb8-78c9-488f-8acf-adba7bb88978b417f193e1eefd01520a624a1f786ec2http://www.researchgate.net/publication/216681389_Goddard_cumulus_ensemble_model._Part_I_Model_descriptionhttp://www.researchgate.net/publication/216681389_Goddard_cumulus_ensemble_model._Part_I_Model_descriptionABSTRACT During the past two decades, convective scale models have advanced sufficiently to study the dynamic and microphysical pro 自由自associated with mesoscale convective systems. The basic features of these models are that they are non-hydrostatic
    Tao, W.-K, J. Simpson, M. McCumber, 1989: An ice-water saturation adjustment. Mon. Wea. Rev., 117, 231- 235.10.1175/1520-0493(1989)1172.0.CO;2e7bc62ff11834766546f8475eda86e05http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F1989MWRv..117..231Thttp://adsabs.harvard.edu/abs/1989MWRv..117..231TABSTRACT A reasonably accurate and noniterative saturation adjustment scheme is proposed to calculate: (1) the amount of condensation and/or deposition necessary to remove any supersaturated vapor, or (2) the amount of evaporation and/or sublimation necessary to remove any subsaturation in the presence of cloud droplets and/or cloud ice. This proposed scheme can be implemented for a nonhydrostatic cloud model. The derivation of the scheme, an evaluation of its performance, and tests for sensitivity to variations in a few key parameters are presented.
    Ueno M., 2007: Observational analysis and numerical evaluation of the effects of vertical wind shear on the rainfall asymmetry in the typhoon inner-core region. J. Meteor. Soc.Japan, 85, 115- 136.10.2151/jmsj.85.115b29f1f16d765a5c77302f0c65c79a9f1http%3A%2F%2Fci.nii.ac.jp%2Fnaid%2F130004434962http://ci.nii.ac.jp/naid/130004434962A number of observational and modeling studies have shown a tendency for typhoon strength vortices to develop upward motion and produce precipitation, particularly in the eyewall, on the downshear to downshear-left side of the tropical cyclones (TCs). However, the directional relationships obtained from the observational studies have been mostly confined to the TC cases in the Atlantic basin. Furthermore, little evidence has been presented so far for the relationship in magnitude, between shear and rainfall asymmetry. In the former part of the present study, the observational analysis on TC rainfall asymmetries is extended to the western North Pacific TCs in 2004, using the two types of rain-rate data, the Radar-AMeDAS precipitation data, and satellite-based rainfall estimates, such as TMI and AMSR-E rain rates. It is well demonstrated from the analysis that rainfall in the inner-core region of a TC tends to occur on the downshear to downshear-left side, irrespective of data type used and latitudes where TCs are located. However, as far as the relationship between shear and storm motion is concerned, a sharp contrast is found between low and middle latitudes. In middle latitudes TCs have a tendency to move to the left of the shear, consistent with previous studies, while in low latitudes they tend to move to the right of the shear. The contrasting shear-relative storm heading between the two latitudes is attributed to the difference in vertical structure of the ambient wind. In the latter part of the study, to explore the quantitative relationship between shear and rainfall asymmetry, a formula for the shear-induced vertical motion is derived from the thermal wind balance equation for TC-like vortices. The formula states that the shear-induced vertical motion should be a function not only of shear magnitude, but also of vortex strength. To validate the formula a set of idealized numerical experiments are conducted, with realistic wind profiles, in which the initial environmental winds are specified from the 6-hourly JMA global analyses for two major typhoon cases in 2004. It is found from the numerical study that the magnitude of wavenumber-one vertical motion, predicted by the formula, is much more strongly correlated with that of model-produced rainfall asymmetry, than the shear alone, suggesting that the vortex strength is one of the main factors determining the magnitude of shear-induced rainfall asymmetry. The results from the idealized simulations also suggest that vortex tilt would have only a minor contribution to the rainfall asymmetry in the inner-core region, at least for well-developed TCs.
    Wang D. H., X. F. Li, W.-K. Tao, and Y. Wang, 2009: Effects of vertical wind shear on convective development during a landfall of severe tropical storm Bilis (2006). Atmospheric Research, 94, 270- 275.10.1016/j.atmosres.2009.06.00463189771-7f84-47ed-af0a-923805a39b0bsdarticleid_3134877d32d6574c188b582b06eb1d9a15e190http%3A%2F%2Fwww.sciencedirect.com%2Fscience%2Farticle%2Fpii%2FS016980950900177Xrefpaperuri:(fed5089b0ec41efb1d7e8943744c2379)http://www.sciencedirect.com/science/article/pii/S016980950900177X<h2 class="secHeading" id="section_abstract">Abstract</h2><p id="">Effects of vertical wind shear on convective development during the landfall of tropical storm Bilis (2006) are investigated with a pair of sensitivity experiments using a two-dimensional cloud-resolving model. The validated simulation data from Wang et al. [Wang, D., Li, X., Tao, W.-K., Liu, Y., Zhou, H., 2009: Torrential rainfall processes associated with a landfall of severe tropical storm Bilis (2006): A two-dimensional cloud-resolving modeling study. Atmos. Res., 91, 94&ndash;104.] are used as the control experiment. The difference between the control and sensitivity experiments is that vertically varying zonal winds in the control experiment are replaced by their mass-weighted means in the sensitivity experiment. The imposed vertical velocity with ascending motion in the upper troposphere and descending motion in the lower troposphere is responsible for dominant stratiform rainfall on 15 July. The vertical wind shear does not have important impacts on development of stratiform rainfall. One day later, imposed upward motion extends to the lower troposphere. The inclusion of negative vertical wind shear produces well-organized convection and strong convective rainfall because it causes kinetic energy transfer from large-scale forcing to perturbation circulations.</p>
    Wu X. Q., M. Yanai, 1994: Effects of vertical wind shear on the cumulus transport of momentum: Observations and parameterization. J. Atmos. Sci., 51, 1640- 1660.10.1175/1520-0469(1994)0512.0.CO;297656cdd4d98051680c01f1340852697http%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F1994JAtS...51.1640Whttp://adsabs.harvard.edu/abs/1994JAtS...51.1640WDynamical effects of organized cumulus convection on its environment with vertical wind shear are studied. Analyses of the wind field and momentum budget residual for mesoscale convective systems observed during SESAME and PRE-STORM reveal systematic differences in the vertical transport of horizontal momentum between mesoscale convective complex (MCC) and squall line cases. In the MCC, a distinct minimum in wind speed appears over the area of intense convection and the momentum budget residual acts to decelerate the environmental wind and to reduce the upper-level vertical shear. Therefore, the inferred vertical transport of momentum in the MCC is downgradient in the upper layer. On the other hand, in the squall line, there is no wind speed minimum and the upper-level vertical shear of the line-normall component of the environmental wind increases as convection develops. Thus, the vertical transport of momentum normal to the squall line is upgradient in the upper layer, although the transport of momentum parallel to the line is downgradient.
    Xu K.-M., A. Arakawa, and S. K. Krueger, 1992: The macroscopic behavior of cumulus ensembles simulated by a cumulus ensemble model. J. Atmos. Sci., 49, 2402- 2420.10.1175/1520-0469(1992)049<2402:TMBOCE>2.0.CO;23e61722b1d7d966c42d1895ad56d0eaehttp%3A%2F%2Fadsabs.harvard.edu%2Fabs%2F1992JAtS...49.2402Xhttp://adsabs.harvard.edu/abs/1992JAtS...49.2402XAbstract The two-dimensional UCLA cumulus ensemble model (CEM), which covers a large horizontal area with a sufficiently small horizontal grid size, is used in this study. A number of simulation experiments are performed with the CEM to study the macroscopic behavior of cumulus convection under a variety of different large-scale and underlying surface conditions. Specifically, the modulation of cumulus activity by the imposed large-scale processes and the eddy kinetic energy (EKE) budget are investigated in detail. In all simulations, cumulus convection is rather strongly modulated by large-scale advective processes in spite of the existence of some nonmodulated high-frequency fluctuations. The modulation exhibits some phase delays, however, when the basic wind shear is strong. This is presumably associated with the existence of mesoscale convective organization. The EKE budget analysis shows that the net eddy buoyancy generation rate is nearly zero for a wide range of cumulus ensembles.
    Zhai G. Q., X. F. Li, P. J. Zhu, H. F. Shen, and Y. Z. Zhang, 2014: Surface rainfall and cloud budgets associated with mei-yu torrential rainfall over eastern China during June 2011. Adv. Atmos. Sci.,31, 1435-1444, doi: 10.1007/s00376-014-3256-7.10.1007/s00376-014-3256-776750cb4bb1877096266f0f7ea9664bahttp%3A%2F%2Fwww.cqvip.com%2FQK%2F84334X%2F201406%2F662244603.htmlhttp://d.wanfangdata.com.cn/Periodical_dqkxjz-e201406018.aspxSurface rainfall and cloud budgets associated with three heavy rainfall events that occurred over eastern China during the mei-yu season in June 2011 were analyzed using 2D cumulus ensemble model simulation data. Model domain mean rainfall showed three peaks in response to three prescribed ascending motion maxima, primarily through the mean moisture convergence during the torrential rainfall period. Prescribed ascending motion throughout the troposphere produced strong convective rainfall during the first(9 June) and third(17-18 June) rainfall events, whereas strong prescribed ascending motion in the mid and upper troposphere and weak subsidence near the surface generated equally important stratiform and convective rainfall during the second rainfall event(14 June). The analysis of surface rainfall budgets reveals that convective rainfall was associated with atmospheric drying during the first event and moisture convergence during the third event. Both stratiform and convective rainfall responded primarily to moisture convergence during the second event. An analysis of grid data shows that the first and third mean rainfall maxima had smaller horizontal scales of the precipitation system than the second.
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Manuscript received: 15 June 2015
Manuscript accepted: 09 November 2015
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Barotropic Processes Associated with the Development of the Mei-yu Precipitation System

  • 1. School of Earth Sciences, Zhejiang University, Hangzhou 310027

Abstract: The barotropic processes associated with the development of a precipitation system are investigated through analysis of cloud-resolving model simulations of Mei-yu torrential rainfall events over eastern China in mid-June 2011. During the model integration period, there were three major heavy rainfall events: 9-12, 13-16 and 16-20 June. The kinetic energy is converted from perturbation to mean circulations in the first and second period, whereas it is converted from mean to perturbation circulations in the third period. Further analysis shows that kinetic energy conversion is determined by vertical transport of zonal momentum. Thus, the prognostic equation of vertical transport of zonal momentum is derived, in which its tendency is associated with dynamic, pressure gradient and buoyancy processes. The kinetic energy conversion from perturbation to mean circulations in the first period is mainly associated with the dynamic processes. The kinetic energy conversion from mean to perturbation circulations in the third period is generally related to the pressure gradient processes.

1. Introduction
  • Barotropic processes represent one of the most important physical process types in the development of precipitation systems. They are described by the kinetic energy conversion between the mean background circulations and perturbation (secondary) circulations associated with vapor condensation and deposition for the production of precipitation. Such kinetic energy conversion is primarily determined by vertical transport of horizontal momentum acting on vertical shear of the mean background horizontal winds (e.g., Pastushkov, 1975). Barotropic processes may affect the development of precipitation systems through the vertical wind shear of background circulations (e.g., Corbosiero and Molinari, 2002; Lang et al., 2007; Ueno, 2007). The vertical wind shear may have impacts on the timing of convection (Xu et al., 1992), the organization of convection (Robe and Emanuel, 2001) and rainfall (e.g, Wang et al., 2009; Shen et al., 2011).

    Severe floods and associated natural disasters occur in the Mei-yu season as torrential rainfall frequently occurs over the middle and lower reaches of the Yangtze River during the early season of the NH summer. (Zhai et al., 2014) conducted a cloud-resolving model study of a Mei-yu heavy rainfall event that occurred over eastern China in mid-June 2011. During the modeling period, there were three major rainfall events, and they found differences in rainfall types and horizontal scale between the three periods. (Wu and Yanai, 1994) revealed the effects of vertical wind shear on the development of a precipitation system through the change in vertical transport of horizontal momentum. But does vertical wind shear determine barotropic kinetic energy conversion directly through the change in vertical transport of horizontal momentum? And which physical processes control vertical transport of horizontal momentum?

    The objective of this study is to examine the barotropic processes associated with the Mei-yu precipitation system through analysis of the differences in barotropic processes between three rainfall events using the Mei-yu simulation data from (Zhai et al., 2014). The model, large-scale forcing, and sensitivity experiments are briefly described in section 2. The results are presented in section 3. A summary is given in section 4.

2. Model and experiments
  • The experiment analyzed in this study was conducted by (Zhai et al., 2014) using the 2D version of a cloud-resolving model (Table 1). The model was integrated with imposed large-scale forcing from 0800 LST 9 June to 0800 LST 20 June 2011. The forcing was averaged in a rectangular box of (30°-31°N, 114°-122°E) using NCEP/GDAS data. There are three upward motion centers while westerly winds prevail (Zhai et al., 2014, Fig. 1). The three torrential rainfall events are forced by the three upward motion centers during the model integration period (Fig. 1). The rainbands are better organized in the third rainfall event than in the two previous rainfall events, while the second rainfall event occupies a larger area than the two other rainfall events. Thus, the model integration period is divided into the three sub-periods: 0800 LST 9 June to 0000 LST 13 June (the first period); 0000 LST 13 June to 1200 LST 16 June (the second period); and 1200 LST 16 June to 0800 LST 20 June (the third period). The large-scale forcing is averaged for the three periods and shown in Fig. 2. The averaged vertical profiles show that westerly winds generally increase with increasing height (Fig. 2a). Near the surface, averaged zonal winds are zero in the first period and weak easterly winds in the two other periods. In the upper troposphere, the westerly winds in the first period are stronger than in the third period, whereas they are weaker in the second period. The averaged upward motions prevail in the troposphere and reach their maxima around 8 km (Fig. 2b). Below 10 km, the averaged upward motions in the third period are stronger than in the first period, but they are weaker than in the second period. Above 10 km, the averaged upward motions in the first period are stronger than in the third period, but they are weaker than in the second period. The averaged rain rates are 0.98 mm h-1 in the first period, 1.38 mm h-1 in the second period, and 1.17 mm h-1 in the third period. The rainfall is stronger in the second period than in the two other periods due to stronger upward motions in the second period. The rain rate is about 20% higher in the third period than in the first period, while the upward motions are only slightly stronger in the third period. The difference in vertical wind shear implies barotropic effects on Mei-yu rainfall.

3. Results
  • Following (Li et al., 2002b), barotropic conversion between the mean kinetic energy to perturbation kinetic energy can be symbolically expressed by the sum of \(C_u(\overline K,K')\) and \(C_w(\overline K,K')\), where \begin{equation*} \label{eq1} C_u(\overline{K},K')=-\left[\overline{u'w'}\dfrac{\partial \overline{u}_{o}}{\partial z}\right] ,(1a) \end{equation*} and \begin{equation*} \label{eq2} C_w(\overline{K},K')=-\left[\overline{w'w'}\dfrac{\partial\overline{w}_{o}}{\partial z}\right] ,(1b) \end{equation*} in which u and w are the zonal and vertical components of wind, respectively; an overbar indicates the model domain mean; a prime indicates a perturbation from the model domain mean; the subscript o is an imposed value from NCEP/ GDAS; [·]=$\int_{z_b}^{z_t}$ $\overline\rho$ · dz and ρ is height-dependent air density, z t and z b are the heights of the top and the bottom of the model atmosphere, respectively. \(C_u(\overline K,K')\) and \(C_w(\overline K,K')\) are the barotropic conversions between the mean domain mean kinetic energy (\(\overline K\)) and K', respectively, through vertical transport of zonal momentum acting on the vertical shear of imposed horizontal-mean zonal wind, and vertical transport of vertical momentum acting on the vertical shear of imposed horizontal-mean vertical velocity. Since the calculations from (Wang et al., 2009) and (Shen et al., 2011) indicate \(C_w(\overline K,K')\) is negligible, the barotropic conversion from the mean kinetic energy to perturbation kinetic energy term can be simplified to \begin{eqnarray} C_u(\overline{K},K')&=&-\left[\overline{u'w'}\dfrac{\partial\overline{u}_{o}}{\partial z}\right]\nonumber\\ &=&-\int_{z_{b}}^{z_{t}}\left(\overline{\rho}\overline{u'w'}\dfrac{\partial\overline{u}_{o}}{\partial z}\right)dz -\int_{z_{b}}^{z_{t}}\overline{\rho}\overline{u'w'}d\overline{u}_{o} .(2)\quad \end{eqnarray}

    Figure 1.  Time-zonal distribution of simulated surface rainfall rate (mm h$^{-1}$).

    Figure 2.  Vertical profiles of (a) zonal wind (m s$^{-1}$) and (b) vertical velocity (cm s$^{-1}$) averaged from 0800 LST 9 June to 0000 LST 13 June (red), from 0000 LST 13 June to 1200 LST 16 June (green) and from 1200 LST 16 June to 0800 LST 20 June (blue).

    To examine the contribution from height-dependent kinetic energy conversion to \(C_u(\overline K,K')\), we calculate the vertical profile of barotropic kinetic energy conversion (BKEC), which can be written as: \begin{equation} {BKEC}={BKEC1}\times {BKEC2} ;(3)\quad \end{equation} $$ {BKEC1}=d\overline{u}_o ;(3a) $$ $$ {BKEC2}=-\rho\overline{u'w'} .(3b) $$ Here, BECK1 is the vertical difference in zonal wind, and BKEC2 is the air density weighted covariance between perturbation zonal wind and vertical velocity or vertical transport of zonal momentum. \(C_u(\overline K,K')\) is calculated by vertically integrating BKEC or adding BKEC for all vertical layers in our calculations.

    The calculations of BKEC show that the BKEC is generally negative in the troposphere in the first period (Fig. 3a). In the second period, the BKEC is positive below 4 km but negative above 4 km (Fig. 3b). The BKEC is generally positive from 1 to 9 km (Fig. 3c). Since negative and positive BKEC values indicate kinetic energy conversion from perturbation to mean circulation and from mean to perturbation circulation, respectively, the positive BKEC value denotes a dynamically unstable system and the negative BKEC value represents a dynamically stable system. Thus, the precipitation system is dynamically stable in the first and second periods and dynamically unstable in the third period.

    The BKEC is associated with the vertical shear of imposed zonal wind (BKEC1) and the vertical transport of zonal momentum (BKEC2), which are time-dependent. Thus, the time-mean BKEC (BKEC hereafter) can be decomposed into the two components $$ {BKEC}_{M}={BKEC1}_{M}\times {BKEC2}_{M} , (4a) $$ and $$ {BKEC}_{T}={BKEC1}_{T}\times {BKEC2}_{T} ,(4b) $$ where BKEC1 M and BKEC2 M are the time averages of BKEC1 and BKEC2, respectively, and BKEC1 T and BKEC2 T are the deviations of BKEC1 and BKEC2 from BKEC1 M and BKEC2 M, respectively. In general, BKEC M is out of phase with BKEC T vertically. BKEC M is negative but BKEC T is positive through the troposphere in the first period (Fig. 3a). BKEC is controlled by BKEC M. In the second period, BKEC M is negative from 2 to 8 km (Fig. 3b). BKEC T is negative above 7 km, whereas it is positive below 7 km. The negative BKEC is associated with the negative BKEC T above 8 km and BKEC M from 4 to 8 km. The positive BKEC corresponds to the positive BKEC T below 4 km. In the third period, BKEC M is positive throughout the troposphere (Fig. 3c). BKEC T is negative above 5 km but it is positive below 5 km. The positive BKEC is determined by the positive BKEC M.

    Since BKEC is controlled by BKEC M, the time-mean BKEC1 and BKEC2 are analyzed (Fig. 4). The imposed zonal winds increase with increasing height in the three periods (Fig. 4a). The time-mean vertical wind shear (BKEC1) barely changes in the first period. The time-mean vertical wind shear is similar in the second and third period, except that the vertical wind shear is decreased to zero around 12 km in the second period but around 10 km in the third period. In the second and third period, the vertical wind shear reaches its peak near the surface, reduces in magnitude around 4 km, and reaches a sub-peak at around 8 km. Since the time-mean vertical wind shear has the same sign in all three periods, the differences in BKEC M between the three periods are attributable to the differences in BKEC2. The time-mean BKEC2 changes from negative values (upward zonal-momentum transport) in the first and second period to positive values (downward zonal-momentum transport) in the third period, through a significant increase in positive BKEC2 from the first and second period to the third period (Fig. 4b). Thus, the dynamic stability (BKEC M) of the precipitation system is determined by BKEC2 in this Mei-yu precipitation system.

    Figure 3.  Vertical profiles of barotropic kinetic energy conversion (BKEC; black) and its components (BKEC$_M$, red; BKEC$_T$, blue) averaged (a) from 0800 LST 9 June to 0000 LST 13 June, (b) from 0000 LST 13 June to 1200 LST 16 June, and (c) from 1200 LST 16 June to 0800 LST 20 June. Units: 10$^5$ J s$^{-1}$.

    To further investigate if the vertical wind shear directly affects the BKEC2, or through which physical factors if the vertical wind shear indirectly affects the BKEC2, the tendency equation of BKEC2 is derived from the perturbation momentum equations. Following (Li et al., 2002b), the perturbation momentum equations in the 2D cloud-resolving model can be written by:\begin{eqnarray} \dfrac{\partial u'}{\partial t}&=&-\dfrac{\partial}{\partial x}(2u'\overline{u}_{o}+u'u')-\nonumber\\ &&\dfrac{1}{\overline{\rho}}\dfrac{\partial}{\partial z}\overline{\rho}(w'\overline{u}_{o}\!+\!\overline{w}_{o}u'\!+\!w'u'-\overline{w'u'})\!-\!c_p\dfrac{\partial(\overline{\theta}\pi')}{\partial x} ;(5a)\qquad \end{eqnarray}

    Figure 4.  Vertical profiles of (a) imposed zonal-wind difference in the vertical layer ($d\overline u_o$; BKEC1; m s$^{-1}$) and (b) air density weighted covariance between perturbation zonal wind and vertical velocity ($-\overline \rho\overline u'w'$; BKEC2; 10$^5$ J m$^{-1}$; solid lines) averaged from 0800 LST 9 June to 0000 LST 13 June (black), from 0000 LST 13 June to 1200 LST 16 June (red), and from 1200 LST 16 June to 0800 LST 20 June (blue). In (b), BKEC2 is broken into components for $u'w'>0$ (long-dashed line) and $u'w'<0$ (short-dashed line).

    $$\begin{eqnarray} \dfrac{\partial w'}{\partial t}&=&-\dfrac{\partial}{\partial x}(u'\overline{w}_{o}+\overline{u}_{o}w'+u'w')-\nonumber\\[-0.5mm] &&\dfrac{1}{\overline{\rho}}\dfrac{\partial}{\partial z}\overline{\rho}(2w'\overline{w}_{o}+w'w'-\overline{w'w'})-\nonumber\\[-0.5mm] &&c_p\dfrac{\partial(\overline{\theta}\pi')}{\partial z}+g\left(\dfrac{\theta'}{\theta_0}+0.61q'_v-q'_l\right) .(5b)\qquad \end{eqnarray} \renewcommand\theequation\arabicequation $$ Here, θ is potential temperature, and θ0 is initial potential temperature; π=(p/p o)\kappa and \(\kappa=R/c_p\); R is the gas constant; cp is the specific heat of dry air at constant pressure p, where p o=1000 hPa; qv is specific humidity; and ql is the sum of the mixing ratios of cloud water, raindrops, cloud ice, snow and graupel.

    Multiplying Eq. (5a) by \(-\overline \rho w'\) and Eq. (5b) by \(-\overline \rho u'\), adding the equations nd taking the model domain mean, the tendency equation of BKEC2 (BKEC2 t) can be expressed by \begin{equation} {BKEC2}_{t}={BKEC2}_{d}+{BKEC2}_{p}+{BKEC2}_{b} , (6)\end{equation} where \begin{align} {BKEC2}_{t}=&\dfrac{\partial}{\partial t}{BKEC2}=\dfrac{\partial}{\partial t}(-\overline{\rho}\overline{u'w'}) ,(6a)\\ {BKEC2}_{d}=&\overline{\rho}\overline{w'\dfrac{\partial}{\partial x}(2u'\overline{u}_{o}+u'u')}+\nonumber\\ &\overline{w'\dfrac{\partial}{\partial z}\overline{\rho}(w'\overline{u}_{o}+\overline{w}_{o}u'+w'u')}+\nonumber\\ &\overline{\rho}\overline{u'\dfrac{\partial}{\partial x}(u'\overline{w}_{o}+\overline{u}_{o}w'+u'w')}+\nonumber\\ &\overline{u'\dfrac{\partial}{\partial z}\overline{\rho}(2w'\overline{w}_{o}+w'w')} ,(6b) \end{align}

    \begin{eqnarray} {BKEC2}_{p}&=&c_p\overline{\rho}\overline{w'\dfrac{\partial(\overline{\theta}\pi')}{\partial x}+u'\dfrac{\partial(\overline{\theta}\pi')}{\partial z}}, (6c)\end{eqnarray} and $$ {BKEC2}_{b}=-\overline{\rho}g\overline{u'\left(\dfrac{\theta'}{\theta_o}+0.61q'_v-q'_l\right)} .(6d) $$

    Here, BKEC2 d, BKEC2 p and BKEC2 b are the contributors to BKEC2 t from the processes related to dynamics, the pressure gradient and buoyancy force, respectively. BKEC2 b can be further partitioned into three terms: \begin{align} {BKEC2}_{b1}&=-\overline{\rho}g\overline{u'\dfrac{\theta'}{\theta_{o}}} ;(7a)\\ {BKEC2}_{b2}&=-0.61\overline{\rho}g\overline{u'q'_v} ;(7b)\\ {BKEC2}_{b3}&=\overline{\rho}g\overline{u'q'_l}. (7c)\end{align}

    The tendency budget of BKEC2 is integrated with time and each term in the budget has a contribution to BKEC2. BKEC2 p is largely balanced by BKEC2 d in the three periods, indicating the dominance of the processes related to dynamics and the pressure gradient in determining BKEC2. BKEC2 is at least three orders of magnitude smaller than these dominant terms. Negative values of BKEC2 correspond mainly to those of BKEC2 d below 8 km and BKEC2 p above 8 km in the first period (Fig. 5a), and those of BKEC2 d above 4 km and BKEC2 p below 4 km in the second period (Fig. 5b). The magnitudes of BKEC2 d and BKEC2 p decrease from the first and second periods to the third period (Fig. 5c). In the third period, positive values of BKEC2 are mainly associated with those of BKEC2 p in the lower and upper troposphere and BKEC2 d in the mid troposphere. BKEC2 b1 and BECK2 b2 contribute to negative values of BKEC2 in the first and second periods, whereas BKEC2 b2 contribute to positive values of BKEC2 in the third period.

4. Summary
  • The barotropic processes associated with the development of a Mei-yu precipitation system are investigated through analysis of conversion between perturbation and mean kinetic energy. The data analyzed are from a 2D cloud-resolving model simulation of three Mei-yu torrential rainfall events that occurred over eastern China in mid-June 2011. The calculations of barotropic kinetic energy conversion show that the precipitation system is dynamically stable (with conversion from perturbation to mean kinetic energy) throughout the troposphere, turns to be weakly unstable in the mid and lower troposphere, and eventually becomes dynamically unstable (with conversion from mean to perturbation kinetic energy) throughout the troposphere.

    The vertical wind shear in the simulation period is increased in imposed zonal winds upward, and the magnitude increases in the mid and lower troposphere from the first period to the second period and barely changes from the second period to the third period. The barotropic conversion is determined by vertical transport of zonal momentum acting on the vertical shear of imposed mean zonal wind. Since the upward increase in zonal winds is imposed during the model integration period, the barotropic conversion is controlled by the vertical transport of zonal momentum (vertical zonal-momentum flux or covariance between perturbation zonal wind and vertical velocity). The zonal-momentum flux is changed from upward in the first and second period to downward in the third period, which leads to the change from a dynamically stable system in the first and second period to a dynamically unstable system in the third period.

    Figure 5.  Vertical profiles of BKEC2 (black) and associated contribution from BKEC2$_d$ (red), BKEC2$_p$ (purple), BKEC2$_b1$ (green), BKEC2$_b2$ (blue) and BKEC2$_b3$ (orange) in the BKEC2 budget averaged (a) from 0800 LST 9 June to 1200 LST 10 June, (b) from 0000 LST 13 June to 0000 LST 15 June, and (c) from 1200 LST 16 June to 1500 LST 18 June. Units: 10$^5$ J m$^{-1}$.

    An equation for predicting the vertical transport of zonal momentum is derived based on prognostic equations of perturbation zonal wind and vertical velocity. The tendency of vertical momentum flux is associated with the processes related to dynamics, the pressure gradient and buoyancy force. The budget analysis of vertical momentum flux reveals that the buoyancy term and pressure gradient term are largely balanced and barotropic stability is mainly related to dynamic processes, whereas barotropic instability is generally associated with the processes related to the pressure gradient.

    Since only one torrential rainfall event is analyzed and the cloud-resolving model used is 2D, a 3D model is needed to study different torrential rainfall cases in various climate regimes to validate the results of this study.

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