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Evolution of Instability before and during a Torrential Rainstorm in North China


doi: 10.1007/s00376-015-5080-0

  • NCEP-NCAR reanalysis data were used to analyze the characteristics and evolution mechanism of convective and symmetric instability before and during a heavy rainfall event that occurred in Beijing on 21 July 2012. Approximately twelve hours before the rainstorm, the atmosphere was mainly dominated by convective instability in the lower level of 900-800 hPa. The strong southwesterly low-level jet conveyed the moist and warm airflow continuously to the area of torrential rain, maintaining and enhancing the unstable energy. When the precipitation occurred, unstable energy was released and the convective instability weakened. Meanwhile, due to the baroclinicity enhancement in the atmosphere, the symmetric instability strengthened, maintaining and promoting the subsequent torrential rain. Deriving the convective instability tendency equation demonstrated that the barotropic component of potential divergence and the advection term played a major role in enhancing the convective instability before the rainstorm. Analysis of the tendency equation of moist potential vorticity showed that the coupled term of vertical vorticity and the baroclinic component of potential divergence was the primary factor influencing the development of symmetric instability during the precipitation. Comparing the effects of these factors on convective instability and symmetric instability showed some correlation.
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  • Bennetts D. A., B. J. Hoskins, 1979: Conditional symmetric instability-a possible explanation for frontal rainbands. Quart. J. Roy. Meteor. Soc., 105, 945- 962.10.1002/qj.49710544615d7500367-8625-4dd2-b821-c8b394a9fae9d8c5cc9cddb42f88f0fd15e2c23a33achttp://onlinelibrary.wiley.com/doi/10.1002/qj.49710544615/pdfhttp://onlinelibrary.wiley.com/doi/10.1002/qj.49710544615/pdfABSTRACT In order to study the possible importance of symmetric baroclinic instability in the formation of frontal rainbands, the existing theory is reviewed and the inclusion of the effects of latent heat release attempted. When an atmosphere is rendered symmetrically unstable by latent heat release, it may be said to be conditionally symmetrically unstable. Simple numerical experiments support the extended theory and describe the structure of the finite amplitude cells. These exhibit conditional gravitational instability in preferred linear regions. It is shown that such a gravitational destabilization is possible only when a wet bulb potential vorticity is initially negative. This latter is a necessary and possibly sufficient condition for ‘conditional symmetric instability’ (CSI). Limited comparison with observed frontal rainbands lends some support to the hypothesis that CSI can be a dominant formative mechanism, though more sophisticated numerical modelling and observational studies are required.
    Bennetts D. A., J. C. Sharp, 1982: The relevance of conditional symmetric instability to the prediction of mesoscale frontal rainbands. Quart. J. Roy. Meteor. Soc., 108, 595- 602.10.1002/qj.4971084570733c20c89-3197-468e-97fb-fcb3979f11ef01fcd437c4f77f4cc2e737bdf80d8e5dhttp%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fqj.49710845707%2Fcitedbyrefpaperuri:(3fdbc762226ab81f49ff244800ad41b3)http://onlinelibrary.wiley.com/doi/10.1002/qj.49710845707/citedbyABSTRACT This paper examines the theory of Conditional Symmetric Instability (Bennetts and Hoskins 1979) and considers its relevance to meso-scale frontal rainbands. The theoretical growth rate of the instability is evaluated from synoptic scale data obtained from a numerical forecast model and compared with observations of the horizontal structure of rainfall observed by radar. One case study is presented in detail and a further 44 cases summarized. Rainbands were observed on 80% of the occasions on which they were predicted.
    Charney J. G., 1947: The dynamics of long waves in a baroclinic westerly current. J. Meteor., 4, 135- 162.10.1175/1520-0469(1947)0042.0.CO;27ca0cc30-984d-4f16-9ae5-5249fd0375ffec38cceb1cb5771f96e1fabd0a960fadhttp%3A%2F%2Fwww.ams.org%2Fmathscinet-getitem%3Fmr%3D22136refpaperuri:(f3972097a8eb020607c024c13e96b4ee)http://www.ams.org/mathscinet-getitem?mr=22136Abstract Previous studies of the long-wave perturbations of the free atmosphere have been based on mathematical models which either fail to take properly into account the continuous vertical shear in the zonal current or else neglect the variations of the vertical component of the earth's angular velocity. The present treatment attempts to supply both these elements and thereby to lead to a solution more nearly in accord with the observed behavior of the atmosphere. By eliminating from consideration at the outset the meteorologically unimportant acoustic and shearing-gravitational oscillations, the perturbation equations are reduced to a system whose solution is readily obtained. Exact stability criteria are deduced, and it is shown that the instability increases with shear, lapse rate, and latitude, and decreases with wave length. Application of the criteria to the seasonal averages of zonal wind suggests that the westerlies of middle latitudes are a seat of constant dynamic instability. The unstable waves are similar in many respects to the observed perturbations: The speed of propagation is generally toward the east and is approximately equal to the speed of the surface zonal current. The waves exhibit thermal asymmetry and a westward tilt of the wave pattern with height. In the lower troposphere the maximum positive vertical velocities occur between the trough and the nodal line to the east in the pressure field. The distribution of the horizontal mass divergence is calculated, and it is shown that the notion of a fixed level of nondivergence must be replaced by that of a sloping surface of nondivergence. The Rossby formula for the speed of propagation of the barotropic wave is generalized to a baroclinic atmosphere. It is shown that the barotropic formula holds if the constant value used for the zonal wind is that observed in the neighborhood of 600 mb.
    Eady E. T., 1949: Long waves and cyclone waves. Tellus, 1, 33- 52.10.3402/tellusa.v1i3.8507ffb3527b-735b-480f-a69e-9c2c34771295db89b19bc99767c1a89ac7525c7b4d31http%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1111%2Fj.2153-3490.1949.tb01265.x%2Fabstractrefpaperuri:(7bf56a91e894b596694f28f290093da2)http://onlinelibrary.wiley.com/doi/10.1111/j.2153-3490.1949.tb01265.x/abstractAbstract By obtaining complete solutions, satisfying all the relevant simultaneous differential equations and boundary conditions, representing small disturbances of simple states of steady baroclinic large-scale atmospheric motion it is shown that these simple states of motion are almost invariably unstable. An arbitrary disturbance (corresponding to some inhomogeneity of an actual system) may be regarded as analysed into “components” of a certain simple type, some of which grow exponentially with time. In all the cases examined there exists one particular component which grows faster than any other. It is shown how, by a process analogous to “natural selection”, this component becomes dominant in that almost any disturbance tends eventually to a definite size, structure and growth-rate (and to a characteristic life-history after the disturbance has ceased to be “small”), which depends only on the broad characteristics of the initial (unperturbed) system. The characteristic disturbances (forms of breakdown) of certain types of initial system (approximating to those observed in practice) are identified as the ideal forms of the observed cyclonc waves and long waves of middle and high latitudes. The implications regarding the ultimate limitations of weather forecasting are discussed.
    Gao S. T., 2000: The instability of the vortex sheet along the shear line. Adv. Atmos. Sci.,17, 525-537, doi: 10.1007/s00376-000-0016-7.10.1007/s00376-000-0016-794d30c42-a140-46cc-bf1e-a3f71cb5c5ecd06eff1910a6d0b1fb83489282217338http://link.springer.com/10.1007/s00376-000-0016-7http://en.cnki.com.cn/Article_en/CJFDTOTAL-DQJZ200004002.htmThe traditional Kelvin -Helmholtz notion of studying the shear instability is not suitable for the case associated with shear line with the strong wind shear in the vortex sheet. Since then, the shear instability becomes theinstability of the vortex sheet. If the velocity is induced by the vortex sheet, the inequalities (161 R r + Ri d )> 0 and U(v,t)> U(A(t)) become the criterion of the vortex sheet instability. This criterion indicates that 1) the disposition of environment field restrains the disturbance developing along the shear line. 2) There exist multi—scale interactions in the unstable process of the shear line. The calculation of the necessary condition for the instability is also presented in this paper.
    Gao S. T., Y. S. Zhou, 2001: The instability of the vortex sheet along the horizontal shear line. Acta Meteorologica Sinica, 59, 393- 404. (in Chinese)10.11676/qxxb2001.04384b239d9-9d75-4b63-aa47-91a70fea09555584200149e55e0d413823057cb0fd3263ffa175dahttp%3A%2F%2Fen.cnki.com.cn%2FArticle_en%2FCJFDTOTAL-QXXB200104001.htmrefpaperuri:(592519b0bb7f8da78bf6b2ca759e99ba)http://en.cnki.com.cn/Article_en/CJFDTOTAL-QXXB200104001.htmThe traditional Kelvin-Helmholtz notion of studying the shearinst ability is not suitable to the shear line with the strong horizontal wind shear.For this case,the shear line should be considered as the vortex sheet.Since then,the instability of this kind of the shear line becomes the instability of the vortex sheet rather than the traditional shear instability.If the velocity is induced by the vortex sheet,the in equalities, (1-<i>R<sub>v</sub></i>+<i>R<sub>id</sub></i>)&gt;0 and <i>U(y,t)</i>><i>U(A(t))</i> become the criterion of the vortex sheet instability.This criterion indicates that the disposition of environment field rest rains the disturbance developing along the shearline,there exist multi-scale interactions between this mesoscale disturbance and environment field.The calculation of the necessary condition for the instability is also presented in this paper.
    Hoskins B. J., 1974: The role of potential vorticity in symmetric stability and instability. Quart. J. Roy. Meteor. Soc., 100, 480- 482.10.1002/qj.497100425204ea82b98-7176-49c7-acb8-d922fe463c7fe764bbeeafbfa4e2f804a1b9738cf489http%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fqj.49710042520%2Fcitedbyrefpaperuri:(738d6342269840e395a8ff53268f9579)http://onlinelibrary.wiley.com/doi/10.1002/qj.49710042520/citedbyNo abstract is available for this article.
    Liu L., L. K. Ran, Y. S. Zhou, and S. T. Gao, 2014: Analysis on the instability and trigger mechanism of torrential rainfall event in Beijing on 21 July 2012. Chinese J. Atmos. Sci.,39, 583-595, doi: 10.3878/j.issn.1006-9895.1407.14144. (in Chinese)
    Lu W. S., H. Y. Shao, 2003: Generalized nonlinear subcritical symmetric instability. Adv. Atmos. Sci.,20, 623-630, doi: 10.1007/BF02915505.10.1007/BF029155056cd22b18-dbd3-43ff-97b4-a7bed4dd3a455ec60fab2dff9269fca650ac9443fce0http%3A%2F%2Flink.springer.com%2F10.1007%2FBF02915505refpaperuri:(8bbdd9a6dcb2efca9b8ab3225d7f8432)http://en.cnki.com.cn/Article_en/CJFDTOTAL-DQJZ200304012.htmStarting from nonlinear equations on the f-plane containing frictional dissipation under the Boussinesq approximation, a new kind of generalized energy is proposed as the Lyapunov function, and averages are taken as any functions of (x, z) instead of the commonly-used means of bilinear functions of (x, z), thereby resulting in a new criterion of generalized nonlinear symmetric stability. It shows that not only must the dissipative coefficient be greater than a certain critical value but the initial disturbance amplitude must be synchronously smaller than another marginal value as well. It follows that the latter imposes a crucial constraint on the former, thus leading to the fact that when the amplitude is bigger compared to another critical value, generalized nonlinear subcritical symmetrical instability may occur. The new criterion contributes greatly to the improvement of the previous results of its kind.
    Ran L. K., L. Liu, N. Li, and Y. B. Qi, 2013: The analysis of the potential-divergence wave activity density and its application to typhoon precipitation. Chinese Journal of Geophysics, 56, 3285- 3301. (in Chinese)
    Ran L. K., Y. B. Qi, and S. C. Hao, 2014: Analysis and forecasting of heavy rainfall case on 21 July 2012 with dynamical parameters. Chinese J. Atmos. Sci., 38, 83- 100. (in Chinese)
    Schultz D. M., P. N. Schumacher, 1999: The use and misuse of conditional symmetric instability. Mon. Wea. Rev., 127, 2709- 2732.10.1175/1520-0493(1999)127<2709:TUAMOC>2.0.CO;260deb399-5949-4983-aaaf-fb91013709df078b540fae7c6c1064c263866af6e316http%3A%2F%2Fwww.researchgate.net%2Fpublication%2F236268991_The_Use_and_Misuse_of_Conditional_Symmetric_Instabilityrefpaperuri:(c4198cbcf3217b565ed4284ac82407c8)http://www.researchgate.net/publication/236268991_The_Use_and_Misuse_of_Conditional_Symmetric_InstabilityA commonly employed explanation for single- and multiple-banded clouds and precipitation in the extratropics is slantwise convection due to the release of moist symmetric instability (MSI), of which one type is conditional symmetric instability (CSI). This article presents a review of CSI with the intent of synthesizing the results from previous observational, theoretical, and modeling studies. This review contends that CSI as a diagnostic tool to assess slantwise convection has been, and continues to be, misused and overused. Drawing parallels to an ingredients-based methodology for forecasting deep, moist convection that requires the simultaneous presence of instability, moisture, and lift, some of the misapplications of CSI can be clarified. Many of these pitfalls have been noted by earlier authors, but are, nevertheless, often understated, misinterpreted, or neglected by later researchers and forecasters. Topics include the evaluation of the potential for slantwise convection, the relationship between frontogenesis and MSI, the coexistence of moist gravitational instability and MSI, the nature of banding associated with slantwise convection, and the diagnosis of slantwise convection using mesoscale numerical models. The review concludes with suggested directions for future observational, theoretical, and diagnostic investigation.
    Schultz D. M., J. A. Knox, 2007: Banded convection caused by frontogenesis in a conditionally, symmetrically, and inertially unstable environment. Mon. Wea. Rev., 135, 2095- 2110.10.1175/MWR3400.1b05bd643-c606-4a36-9cb7-431438e3bb752f4702a77e70cd58f39f40bb12559b2ehttp%3A%2F%2Fwww.researchgate.net%2Fpublication%2F252408854_Banded_Convection_Caused_by_Frontogenesis_in_a_Conditionally_Symmetrically_and_Inertially_Unstable_Environmentrefpaperuri:(e3911dea003d2f4884d1a04eb4ad5e8c)http://www.researchgate.net/publication/252408854_Banded_Convection_Caused_by_Frontogenesis_in_a_Conditionally_Symmetrically_and_Inertially_Unstable_EnvironmentAbstract Several eastest-oriented bands of clouds and light rain formed on 20 July 2005 over eastern Montana and the Dakotas. The cloud bands were spaced about 150 km apart, and the most intense band was about 20 km wide and 300 km long, featuring areas of maximum radar reflectivity factor of about 50 dB Z . The cloud bands formed poleward of an area of lower-tropospheric frontogenesis, where air of modest convective available potential energy was being lifted. During initiation and maintenance of the bands, mesoscale regions of dry symmetric and inertial instability were present in the region of the bands, suggesting a possible mechanism for the banding. Interpretation of the extant instabilities in the region of the bands was sensitive to the methodology to assess the instability. The release of these instabilities produced circulations with enough vertical motion to lift parcels to their lifting condensation level, resulting in the observed cloud bands. A high-resolution, numerical weather prediction model demonstrated that forecasting these types of events in such real-time models is possible, although the timing, evolution, and spacing of the bands were not faithfully reproduced. This case is compared to two previous cases in the literature where banded convection was associated with a combination of conditional, symmetric, and inertial instability.
    Seltzer M. A., R. E. Passarelli, and K. A. Emanuel, 1985: The possible role of symmetric instability in the formation of precipitation bands. J. Atmos. Sci., 42, 2207- 2219.10.1175/1520-0469(1985)042<2207:TPROSI>2.0.CO;2d9accc16-e0a6-4b2e-b06d-26bd610b292933bb4da1e34ca3501da4da4fddfe7257http%3A%2F%2Fwww.researchgate.net%2Fpublication%2F253468676_The_Possible_Role_of_Symmetric_Instability_in_the_Formation_of_Precipitation_Bandsrefpaperuri:(5232728ffdda787e2377c9bd701d76ca)http://www.researchgate.net/publication/253468676_The_Possible_Role_of_Symmetric_Instability_in_the_Formation_of_Precipitation_BandsAbstract Fifteen cases of banded and nonbanded precipitation not associated with surface frontal regions are presented. Results from the linear perturbation and parcel theories of symmetric instability are compared to the observed properties of these bands. Symmetric instability can explain many of the features of the bands considered in this study: all of the bands are aligned parallel to the thermal wind; strong shear and near-neutral static stabilities are observed when bands occur; multiple bands have a wavelength that is related to the depth of the unstable region and the slope of moist isentropic surfaces. However, the linear theory of symmetric instability assumes a basic state of unidirectional flow and thermal wind balance, while the observations indicate that in some cases these conditions are not met. This study supports the hypothesis that symmetric instability may be responsible for precipitation bands, but the comparison between theory and observations is hampered by the inability of the pre...
    Seman C. J., 1994: A numerical study of nonlinear nonhydrostatic conditional symmetric instability in a convectively unstable atmosphere. J. Atmos. Sci., 51, 1352- 1371.2169d519-10ef-4a0b-a6dd-e4618ec0ab04307345e47a9a7e50554f353b625b8c72http%3A%2F%2Fconnection.ebscohost.com%2Fc%2Farticles%2F9501202770%2Fnumerical-study-nonlinear-nonhydrostatic-conditional-symmetric-instability-convectivelyrefpaperuri:(2463d0426c5908d3235b110a0e6636b6)http://connection.ebscohost.com/c/articles/9501202770/numerical-study-nonlinear-nonhydrostatic-conditional-symmetric-instability-convectivelyStudies nonlinear hydrostatic conditional symmetric instability (CSI) as an initial value problem. Use of a two-dimensional, nonlinear, nohydrostatic mesoscale/cloud model; Simulation of the rotating baroclinic field (BCF); Enhancement of mesoscale circulation growth by baroclinicity.
    Stone P. H., 1966: On non-geostrophic baroclinic stability. J. Atmos. Sci., 23, 390- 400.10.1175/1520-0469(1966)023<0390:ONGBS>2.0.CO;2d505b00a-aee0-4e7e-a523-c1a0aea6676448ce6609e32b2cb503ef15f6cd16f9a0http%3A%2F%2Fwww.researchgate.net%2Fpublication%2F234236233_On_Non-Geostrophic_Baroclinic_Stabilityrefpaperuri:(a650a5c230442c57a61dea3fa72661a5)http://www.researchgate.net/publication/234236233_On_Non-Geostrophic_Baroclinic_StabilityAbstract Eady's (1949) model is used to study the non-geostorphic baroclinic stability problem. Growth rates for various types of perturbations are found as a function of the Richardson number, Ri The results indicate that the conventional baroclinic instabilities dominate if Ri > 0.95; symmetric instabilities dominate if 1/4 Ri > 0.95; and symmetric instabilities dominate if Ri < 1/4. It is suggested that symmetric instabilities may play an important role in the dynamics of the atmospheres of the major planets of the solar system.
    Stone P. H., 1970: On non-geostrophic baroclinic stability: Part II. J. Atmos. Sci., 27, 721- 726.10.1175/1520-0469(1970)0272.0.CO;20d427c46-b9da-463a-9f89-6ee3c05d71134fe157bc2f6d3011628858b100a0c70ehttp%3A%2F%2Fwww.researchgate.net%2Fpublication%2F253716804_On_Non-Geostrophic_Baroclinic_Stability_Part_IIrefpaperuri:(5428cbf99955c01f244936f740873130)http://www.researchgate.net/publication/253716804_On_Non-Geostrophic_Baroclinic_Stability_Part_IIAbstract The solutions of Eady's 1949 model of baroclinic stability are extended numerically to include the non-geostrophic perturbations which wore not covered by the analysis in Part I. It is found that the largest growth rates are never associated with these new perturbations, so the tentative conclusions of Part I are verified. The more exact numerical solutions lead only to slight quantitative modifications of the results of Part I. If we let Ri be the Richardson number, then the largest growth rates are associated with “geostrophic” baroclinic instability if Ri>0.950; with symmetric instability if 04<Ri<0.950; and with Kelvin-Helmholtz instability if 0<Ri<04. Geostrophic baroclinic instability and symmetric instability can exist simultaneously if 0.84<Ri<1, and symmetric instability and Kelvin-Helmholtz instability can exist simultaneously if 0<Ri<04
    Stone P. H., 1971: Baroclinic stability under non-hydrostatic conditions. J. Fluid Mech., 45, 659- 671.
    Sun J. S., N. He, R. Guo, and M. X. Chen, 2013a: The configuration change and train effect mechanism of multi-cell storms. Chinese J. Atmos. Sci., 37, 137- 148. (in Chinese)fe0bb921-635f-4fc9-8488-1390ae5af800a08535cd253d9eda8ac8f07544d692cfhttp://en.cnki.com.cn/Article_en/CJFDTOTAL-DQXK201301014.htmhttp://en.cnki.com.cn/Article_en/CJFDTOTAL-DQXK201301014.htmSeveral multi-cell storm systems occurring in the Beijing area have been investigated by using the low-level thermal and dynamical retrieval system of four-dimensional variational assimilation (4Dvar) based on the Variational Doppler Radar Analysis System (VDRAS). This paper examines the physical mechanism of configuration processes, intensity changes, and train-effect phenomena that occur during the transmission of linear multi-cell storms. The following results are reported: (1) In a multi-cell storm system in which the transmission direction of the cells is constant with a convective band such as a squall line, the configuration changes such that linear reflectivity becomes arched, and intensity changes of the cells are related to interaction of cells transmitting process and environmental low-level air flow. If the frontal inflow is a warm and moist air stream, and stronger vapor convergence is present, the cell flourishes more easily and transmits faster; otherwise, the cell weakens and transmits slowly. Therefore, in squall-line system nowcasting, the intersection of the multi-cell transmitting direction and the environmental vapor convergent line should be closely followed because the cell will travel faster, and the most severe effects of convection will occur. (2) In a multi-cell system that shows characteristics of a train effect, the cell transmitting feature and developing environment differ almost completely from those of the multi-cell previously mentioned. Train-effect phenomena generally occur in low-level warm and moist air streams or neighboring low-level jets in unstable ambient atmospheric conditions. The transmitting mechanism of the storm cell can be connected with the propagation and stimulation of an inertial gravity wave such that the warm and moist air stream or low-level jet is a transmitting band for warm vapor advection. When inertial gravity wave propagates from high to lowse , the wave receives energy from the ambient atmosphere and develops constantly. Therefore, during storm cell transmission, cells gradually enhance and become arranged in a row to produce the torrential rain center in the leading end of the wave train.
    Sun J. H., S. X. Zhao, S. M. Fu, H. J. Wang, and L. L. Zheng, 2013b: Multi-scale characteristics of record heavy rainfall over Beijing area on July 21, 2012. Chinese J. Atmos. Sci., 37, 705- 718. (in Chinese)f3144b5d-00c8-4d3a-9758-50549dd1370f1b9e0c412ac05bfa490cf3cf0cacc5f7http%3A%2F%2Fen.cnki.com.cn%2FArticle_en%2FCJFDTOTAL-DQXK201303014.htmrefpaperuri:(a4de56f9134485b4ec693e7bbb61fc79)http://en.cnki.com.cn/Article_en/CJFDTOTAL-DQXK201303014.htmObservational and National Centers for Environmental Prediction (NCEP) analysis data are used to diagnose the characteristics of synoptic circulations, sources of water vapor, and mesoscale convective systems (MCS) related to the formation of heavy rainfall on July 21, 2012. Results indicate that the locations and intensities of upper-to lower-level synoptic circulations and mid-to low-latitude systems are favorable for the heavy rainfall formation over North China that occurred under typical weather patterns with high pressure to the east and low pressure to the west. Synoptic systems such as vortices, shear lines, troughs, cold fronts, and low-level jets affect the formation and intensity of heavy rainfall. Tropical cyclones in the Bay of Bengal and the western Pacific Ocean provide favorable conditions for the transportation of water vapor from the ocean to the mainland. The sources of water vapor to North China are the Bay of Bengal, the Bohai Sea, and the Yellow Sea. Water vapor in the lowertroposphere is mainly transported from the latter two sources, and water vapor in the middle troposphere is mainly transported from the former. The entire heavy rainfall process involves two stages. During the first stage, the trigger-ing of MCS is associated with cold air invasion, terrain, and easterly wind in the prefrontal area. During the second stage, the organization and intensification of MCS are forced by the cold front. Under favorable synoptic circulations, the frequent development of stable and persistent MCS is important for the formation of the heavy rainfall event ex- amined in this study.
    Wang J. Y., C. G. Cui, X. F. Wang, and W. J. Cui, 2014: Analysis on water vapor transport and budget of the severe torrential rain over Beijing Region on 21 July 2012. Meteorological Monthly, 40, 133- 145. (in Chinese)bab86408-1d8c-414c-b672-d0d0de0f53efcf7e92cce1037e043cec5e98a1a26027http%3A%2F%2Fen.cnki.com.cn%2FArticle_en%2FCJFDTotal-QXXX201402001.htmhttp://en.cnki.com.cn/Article_en/CJFDTotal-QXXX201402001.htmBy using the NCEP reanalysis data,the vapor budget of the area covered by the severe torrential rain over the northeast of North China on 21 July,2012 is calculated according to the vapor budget equation.The results show that meridional water vapor transportation is dominant while the extremely heavy rain hits Beijing Region,where most moist vapor comes from the southern boundary below 500 hPa.The low-level regional moisture convergence is consistent with the time and space when the torrential rain breaks out and develops.Above the middle level the vertical vapor transport is more prominent.Then the variation features of the vapor transport corridors and their moisture contributions are got through the HYSPLIT mode.The backward trajectory analyses illustrate two major vapor transport corridors.The moistest vapor derived from Yellow Sea and East China Sea along the low level make the main moisture contribution during the heavy precipitation.Moisture from the South China Sea and the Bay of Bengal strengthens the water vapor in the region when the heavy rain starts and develops.Also the drier vapor corridor along the high level from the northwest of China plays an important role in this case.
    Wu G. X., Y. P. Cai, and X. J. Tang, 1995: Moist potential vorticity and slantwise vorticity development. Acta Meteorologica Sinica, 53, 387- 405. (in Chinese)10.11676/qxxb1995.045291d7ed5-b168-43f7-8026-b290436c322155841995467ee25f9c92a212174f27e57fc92a5cdchttp%3A%2F%2Fen.cnki.com.cn%2FArticle_en%2FCJFDTOTAL-QXXB504.001.htmrefpaperuri:(30cd25d1f715e380ba4f8cdaf997c49b)http://en.cnki.com.cn/Article_en/CJFDTOTAL-QXXB504.001.htmAn accurate form of the moist potential vorticity (MPV) equation was deduced from a complete set of primitive equations system.It was shown that motion in a saturated atmosphere without diabatic heating and frictional dissipation conserves moist potential vorticity. This property was then used to investigate the development of vertical vorticity in moist baroclinic Processes.Results show that in the frame work of moist isentroPic coordinate,vorticity development can result from reduction of convective stability,or convergence,or latent heat release in isentropic surfaces.However,the application of the usual analysis of moist isentropic potential vorticity 15 limitted due to the declination of moist isentropic surfaces,and atheory of slantwise vorticity development based on <i>Z</i>-coordinate and <i>P</i>-coordinate was then proposed. According to this theory,whether the atmosphere 15 moist symetrically stable or unstable,or convectively stable or unstable,50 long as the moist insentropic surface 15 slantwise the reduction of convective stability,the increase of the vertical shear of horizontal wind or moist baroclinity can result in the increase of vertical vorticity.The larger the declination of the moist isentropes,the more vigorous the deveolopment of vertical vorticity.Ina region with a monsoonal front to the north and warm and moist air to the south,or bye the north of front the moist isentropes are very stiff.This 15 the region most favorable for the develoPment of vorticities and formation of torrential rain. For a case of Persistent torrential rain occuriny in the middle and lower reaches of the Yangtze and Huai River in June 12-15,1991,moist potential vorticity analysis,especially the isobaric analysis of its vertical and horizontal compoments,i e.MPVI and MPVZ respectively,is effective for inaentifying synoptic systems not only in middle and high latitudes,but also in the low latitudes and in the lower troposphere.It can serve as a powerful tool for the diagnosis and Prediction of torrential rain.
    Wu G. X., Y. P. Cai, 1997: Vertical wind shear and down-sliding slantwise vorticity development. Scientia Atmospherica Sinica, 21, 273- 282. (in Chinese).a02ae177-78f8-4414-8b26-a17e8ef957ac3264bb0d0cc3320d8fc739bb4fbf22e7http%3A%2F%2Fen.cnki.com.cn%2FArticle_en%2FCJFDTOTAL-DQXK703.002.htmrefpaperuri:(0508272d745c3c216b90db8661851796)http://en.cnki.com.cn/Article_en/CJFDTOTAL-DQXK703.002.htmBased upon the conservation property of moist potential vorticity ( P m ) of an adiabatic, frictionless, and saturated atmosphere, the development of vertical vorticity in a moist baroclinic process was discussed. When moist isentropic surfaces are tilted, the application of the traditional “isentropic potential vorticity” (IPV) analysis is limited. A theory of slantwise vorticity development was then developed to investigate the vorticity intensification from a Lagrangian point of view. It was shown that in the area between the south of monsoon front and the north of warm and moist air mass, moist isentropic surfaces are stiff. This area then becomes a favorable region for the development of cyclone and torrential rain. The necessary condition and sufficient condition for slantwise vorticity development are discussed. It is proved that in a convectively unstable and saturated atmosphere, the occurence of slantwise vorticity development must be accompanied by the existence of a low level jet. Application of this theory to a case analyses of typical monsoonal torrential rain shows that the P m analysis, especially the analysis of P m1 (=- g(f+ζ p) θ e/ p) and P m2 (=- g× / p· pθ e ) at isobaric surfaces in the lower troposphere, is very effective in identifying the occurence of torrential rain, and may be used as a powerful tool for the diagnosis and prediction of torrential rain.
    Wu G. X., H. Z. Liu, 1999: Complete form of vertical vorticity tendency equation and slantwise vorticity development. Acta Meteorologica., 57, 1-15. (in Chinese)05e7eeb5-e779-4c47-af41-c641ded384213a4ae8ab7aaa06a6a60283e350722c66http%3A%2F%2Fwww.cmsjournal.net%2Fqxxben%2Fch%2Freader%2Fview_abstract.aspx%3Ffile_no%3D19990101%26flag%3D1refpaperuri:(8305a2d5ef2cd822f2580a8c8c3d226c)http://www.cmsjournal.net/qxxben/ch/reader/view_abstract.aspx?file_no=19990101&amp;flag=1
    Xu Q., 1986: Conditional symmetric instability and mesoscale rainbands. Quart. J. Roy. Meteor. Soc., 112, 315- 334.10.1002/qj.497112472037d2abe80-a047-4133-b7cc-2ff6cb92a56f584b3b697072b6375b95ed47ccbb43b1http%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1002%2Fqj.49711247203%2Fcitedbyrefpaperuri:(53ac4b2c0f8888842ec0b819d471ff5c)http://onlinelibrary.wiley.com/doi/10.1002/qj.49711247203/citedbyABSTRACT The linear theory of conditional symmetric instability (CSI) is re-examined in a rigorous framework. In comparison with symmetric instability a new feature of CSI is that the moist updraught tends to be narrow, as with conditional buoyancy instability (CBI). As the width of the moist updraught varies from its tolerance maximum to infinitesimal, the inviscid growth rate increases from zero to its maximum and the slope of the moist updraught increases from the absolute momentum surface to the moist most unstable surface. The fact that CSI circulations absorb energy from the basic shear and moist thermal field but lose energy to the dry basic thermal field is responsible for the narrow and slant feature of the moist updraught. When a bulk viscosity is accounted for, the most rapidly growing CSI modes bear a qualitative resemblance to some observed rainbands. The stability criterion of viscous CSI also shows a better comparison with observational data than inviscid CSI. The linear CSI theory here predicts that the isolated mode is preferred to other non-isolated (periodic or irregular spacing) modes. The preference of non-isolated modes is speculated to occur in the nonlinear stage.
    Zhang K. S., 1988a: On mesoscale instability of a baroclinic flow 1. Symmetric instability. Acta Meteorologica Sinica, 46, 258- 266. (in Chinese)10.11676/qxxb1988.033b1b81971-f7c8-4474-a830-cbc4cd19190e558419883175bb6c42e31366f46dea1d61836b0a9b7http://en.cnki.com.cn/Article_en/CJFDTOTAL-QXXB198803001.htmhttp://en.cnki.com.cn/Article_en/CJFDTOTAL-QXXB198803001.htmThe first part of the present work investigates instability of a baroclinic basic flow against the mesoscale disturbances parallel to it. The focus of this study is to search for the possibility for a mesoscale disturbance of band structure to occur in a stably stratified atmosphere and its effect on triggering and organizing deep convections,The two- and three-dimensional perturbation equations, suitable to solving eigenvalue problems by use of the generalized matrix method and shooting method, are formed under anelastic approximation. The criteria for symmetric instability to set in are discussed for a linear, a hyperbolic-tangential and a real wind profile sounded before occurrence of a squall line event in SESAME 1979. The effect of baroclinicity of the basic flow on occurrence of this kind inertial convection is also analyzed in terms of energetic calculation.
    Zhang K. S., 1988b: On mesoscale instability of a baroclinic flow 2. transversal instability. Acta Meteorologica Sinica, 46, 385- 392. (in Chinese)10.11676/qxxb1988.0503d437f56-d9f9-432a-89d0-014cd2fe3a1a558419884122aa87948168308b9fbb3af124a6c9cc6http%3A%2F%2Fen.cnki.com.cn%2Farticle_en%2Fcjfdtotal-qxxb198804000.htmrefpaperuri:(587a19634e5bb3343173431800e86dc5)http://en.cnki.com.cn/article_en/cjfdtotal-qxxb198804000.htmThe second part of the present study investigates instability of a baroclinic basic flow against the transversal mesoscale disturbances. By generalizing the Eady model to an ageostrophic one, the bi-mode and even mufti-mode instability spectra may occur for a baroclinic basic flow. The Eady-mode appears at synoptic scales, whereas the ageostrophic, baroclinic mode appears at inertial scales ranging from sevenal tens to hundreds kinometers. The Eady-mode, with a qrasi-geostrophic structure, has a larger vertical depth, while the meso-modes are mostly confined to the middle and lower troposphere with an asymmetric "cat eyes" pattern in the vertical cross section and an alternative distribution of divergence and vorticity in the horizontal plane. The growth rate of the mesoscale mode is about four times larger than that of the Eady-mode for the same wind profile of linear distribution. the major energy source, which supports these two modes, is the baroclinic available potential energy stored in a rotating basic flow. The results of this paper may be useful in analysis of the mesoscale distur-bances'propagating along a basic flow.
    Zhang L. F., M. Zhang, 1992: Wave-CISK and symmetric instability. Scientia Atmospherica Sinica, 16, 669- 676. (in Chinese)717634e8-e607-4f5c-94d1-e3861f0d48a29ca90fda497bc26986045473c01faddfhttp%3A%2F%2Fen.cnki.com.cn%2FArticle_en%2FCJFDTOTAL-DQXK199206003.htmrefpaperuri:(66c526c0c38ec8aa2833343e03afae3b)http://en.cnki.com.cn/Article_en/CJFDTOTAL-DQXK199206003.htmIn this paper the symmetric instability is studied when the condensation heating existing. The wave-CISK parameterized scheme is used in the convection condensation heating term. The calculation results show that the disturbance, of propagating symmetric instability is produced through CISK mechanism and the propagating direction, the growing rate and the structure of disturbance are affected by convection condensation heating.
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Manuscript received: 23 March 2015
Manuscript revised: 31 May 2015
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Evolution of Instability before and during a Torrential Rainstorm in North China

  • 1. Institute of Atmospheric Physics, Chinese Academy Sciences, Beijing 100029
  • 2. Graduate University of Chinese Academy of Sciences, Beijing 100040
  • 3. State Key Laboratory of Severe Weather, Chinese Academy of Meteorological Sciences, Beijing 100081

Abstract: NCEP-NCAR reanalysis data were used to analyze the characteristics and evolution mechanism of convective and symmetric instability before and during a heavy rainfall event that occurred in Beijing on 21 July 2012. Approximately twelve hours before the rainstorm, the atmosphere was mainly dominated by convective instability in the lower level of 900-800 hPa. The strong southwesterly low-level jet conveyed the moist and warm airflow continuously to the area of torrential rain, maintaining and enhancing the unstable energy. When the precipitation occurred, unstable energy was released and the convective instability weakened. Meanwhile, due to the baroclinicity enhancement in the atmosphere, the symmetric instability strengthened, maintaining and promoting the subsequent torrential rain. Deriving the convective instability tendency equation demonstrated that the barotropic component of potential divergence and the advection term played a major role in enhancing the convective instability before the rainstorm. Analysis of the tendency equation of moist potential vorticity showed that the coupled term of vertical vorticity and the baroclinic component of potential divergence was the primary factor influencing the development of symmetric instability during the precipitation. Comparing the effects of these factors on convective instability and symmetric instability showed some correlation.

1. Introduction
  • A torrential rain event occurred over Beijing and Hebei Province in China on 21 July 2012. Being the most severe event of the past 60 years, it attracted great attention. Its strength exceeded expectations, and it caused major losses of life and property. Many researchers have analyzed the mechanism of this extreme event from different points of view. (Sun et al., 2013a) found that the train-effect phenomenon was obvious during the precipitation, and connected it with the propagation of an inertial gravity wave. (Sun et al., 2013b) explored the effect of the interaction of multi-scale weather systems on the torrential rain over Beijing. (Wang et al., 2014) analyzed the water vapor transport features over Beijing. (Ran et al., 2014) developed a dynamical element forecast equation with the moist thermodynamic advection parameter, the convective vorticity vector, the thermodynamic wave-activity density, and so on, to predict the torrential rain. However, these previous studies focused mainly on the circulation structure, vapor conditions or multi-scale interactions, while relatively few studies have examined the physical mechanism of the instability evolution. Strengthening the analysis on the physical mechanism of instability is important and helpful for improving understanding of the generation and development of torrential rain.

    Scholars both home and abroad began researching instability and precipitation many years ago. (Charney, 1947) and (Eady, 1949) put forward the idea of baroclinic instability and used it to explain the constant dynamic instability of midlatitude westerly flow. Stone (1966, 1970, 1971) explored the baroclinic instability in the non-geostrophic atmosphere, and then (Hoskins, 1974) noted that symmetric instability was one of the trigger mechanisms for frontal rainfall. (Bennetts and Hoskins, 1979) found that the perturbation of mesoscale symmetric instability played a significant role in organizing precipitation. By investigating the relationship between symmetric instability and precipitation, (Seltzer et al., 1985) proved that symmetric instability was an important mechanism for the formation of precipitation. (Xu, 1986) re-examined the linear theory of conditional symmetric instability in a rigorous framework and proposed two types of conditional symmetric instability. Zhang (1988a, b) investigated symmetric instability and transversal instability in baroclinic basic flow and explored the effect of baroclinicity on ageostrophic inertial flow. (Wu et al., 1995), (Wu and Cai, 1997), (Wu and Liu, 1999) diagnosed the conditional symmetric instability with the moist potential vorticity (MPV) and found that the slant of the moist isentropic surface caused by the enhanced vertical wind shear or the increased horizontal moist baroclinic wind would strengthen the vertical vorticity, thus causing heavy rainfall. (Zhang and Zhang, 1992) researched the influence of the wave-CISK (conditional instability of the second kind) mechanism on symmetric instability and revealed the feature of symmetric instability perturbation. In the actual atmosphere, convective instability often occurs simultaneously with symmetric instability. (Seman, 1994) proposed the theory of nonlinear convective-symmetric instability. (Schultz and Schumacher, 1999) reviewed the applicability of symmetric instability to various atmospheric situations. (Gao, 2000) and (Gao and Zhou, 2001) hypothesized that when the horizontal wind shear is strong the shear line becomes the instability of the vortex sheet rather than the traditional shear instability. Starting from nonlinear equations containing frictional dissipation under the Boussinesq approximation, (Lu and Shao, 2003) proposed a new type of generalized energy, resulting in a new criterion of generalized nonlinear symmetric instability. (Schultz and Knox, 2007) explored the relationship between banded convection and a combination of conditional, symmetric and inertial instability. Based on the aforementioned work, the theory of atmospheric instability has been widely applied to weather analysis, and great progress has been made.

    Building on previous research, this study aims to explore the characteristics and evolution mechanism of instability before and during a precipitation event that occurred in Beijing on 21 July 2012, in the hope of providing significant insight for further heavy rainfall of a similar nature. Section 2 introduces the background situation of the case and the characteristics of the precipitation. Section 3 analyzes the convective and symmetric instability in detail. Section 4 deduces the tendency equation of convective instability and examines the effect of various elements on the convective instability before the precipitation. Section 5 deduces the tendency equation of symmetric instability and discusses its variation during the precipitation. Section 6 summarizes the key conclusions of the study.

2. An observational overview of the squall line and its environment
  • During the period 21-22 July 2012 a torrential precipitation event occurred over northern China. The heavy rainfall occurred at about 0200 UTC and had generally vanished by 1800 UTC 21 July. The rain band was oriented from southwest to northeast (Fig. 1). The center of the precipitation was over Beijing (40°N, 116°E) and northern Hebei Province, where the 24-h accumulated precipitation reached 200 mm. Before 0800 UTC 21 July there was precipitation generated in the warm region in the front of the front. The center of precipitation scattered. Then, after 0800 UTC 21 July, the front moved into the Beijing area, and the scattered center gradually organized into a marked rain band oriented from southwest to northeast.

    In this study, the period before and during the precipitation were both considered to explore the evolution of the instability.

    Figure 1.  The 24-h accumulated precipitation (units: mm) from 0000 UTC 21 to 0000 UTC 22 July. The black box represents the location of Beijing (39.5$^\circ$-41$^\circ$N, 115.5$^\circ$-117.3$^\circ$E).

  • In this study, global forecast system (GFS) reanalysis data from the National Centers for Environment Prediction (NCEP) were used to calculate and explore the spatial and temporal evolution of atmospheric instability and its physical mechanism. The GFS data were collected at four times (0000, 0600, 1200 and 1800 UTC), with a horizontal resolution of 0.5°×0.5° and a vertical resolution of 26 levels.

    The precipitation formed in an environment with a well-defined trough, surface shear line, low-level jet, high-level jet, and sufficient moisture. At 500 hPa (Fig. 2a), the westerly wind trough was located over Lake Baikal; meanwhile, there were ridges at Barr Kersh Lake (60°-90°E) and eastern Asia, forming a "two ridge and one trough" environment. The 588 (gpm) line of the subtropical high jumped from 33°N to 36°N, shaping a "high-pressure dam", which typically favors an "east-high-west-low" situation for northern torrential precipitation. At the moment of the storm's approach (0000 UTC 21 July), the westerly wind trough merged with another trough over northwestern China, moving into northern China. There was a wide range of southwesterly warm and moist airflow in front of the trough impacting on Beijing (40°N, 116°E) and Hebei Province. At 1200 UTC 21 July (Fig. 2b), the 588 (gpm) line of the subtropical high maintained stability, blocking the westerly trough from moving eastward, and thus the system was detained over northern China, causing the persistent precipitation.

    Figure 2.  The distribution of (a) geopotential height at 500 hPa (red line; units: gpm) and wind vector (units: m s$^-1$) at 1200 UTC 20 July; (b) geopotential height at 500 hPa (red line; units: gpm) and wind vector (units: m s$^-1$) at 0600 UTC 21 July; (c) geopotential height at 700 hPa (black line; units: gpm), the low-level jet at 850 hPa (shaded) and positive relative vorticity (red line; units: 10$^-4$ s$^-1$) at 0000 UTC 21 July; (d) geopotential height at 700 hPa (black line; units: gpm), the low-level jet at 850 hPa (shaded) and positive relative vorticity (red line; units: 10$^-4$ s$^-1$) at 0600 UTC 21 July; (e) wind vector (units: m s$^-1$) and the high-level jet (shaded) at 200 hPa at 1200 UTC 21 July; and (f) relative humidity (shaded) and wind vector (units: m s$^-1$) at 925 hPa at 1200 UTC 21 July.

    At 700 hPa, before the heavy rainfall, the low-level trough over northwestern China moved eastward along with steering flow. At the moment of the storm's approach (0000 UTC 21 July), the low-level trough developed intensively and formed a closed vortex. At 0600 UTC, the vortex moved to Beijing. The southwesterly airflow in front of the trough increased, reaching 16 m s-1. At 1200 UTC 21 July (Fig. 2d), the vortex was over the Beijing area and the low-level jet had enhanced, reaching 20 m s-1. Beijing was located on the left side of the exit of the low-level jet. There was strong cyclonic shear and upward motion over the Beijing area. At 200 hPa (Fig. 2f), from 0600 UTC to 1800 UTC 21 July, the Beijing area was at the entrance of the high-level jet, where there was strong divergence. In accordance with the low-level jet, there was a favorable situation of divergence at the high level, and convergence at the low level, over northern China.

    Figure 3.  Vertical distribution (hPa) of pseudo-equivalent potential temperature ($\theta_ se$; contours; units: K) and vertical velocity (shaded; units: hPa s$^-1$) along 40$^\circ$N at (a) 1800 UTC 20 July and (b) 1200 UTC 21 July. (c) Temporal evolution (UTC) of the vertical gradient of pseudo-equivalent potential temperature (shaded; units: K) and 6-h accumulated precipitation (line; units: mm). (d) Temporal evolution (UTC) of vorticity (contours; 10$^-5$ s$^-1$) and divergence (shaded; units: 10$^-5$ s$^-1$) over the Beijing area (39.8$^\circ$-40.0$^\circ$N, 115.8$^\circ$-116.2$^\circ$E).

    Figure 2g shows the vapor conditions at 850 hPa. The main water vapor channel was from the Bay of Bengal, transported by a strong southwesterly low-level jet. Furthermore, there was another channel from the South China Sea, which was transported by the southeasterly wind formed between the tropical storm "Vicente" and the subtropical high. These two primary channels provided sufficient vapor for the heavy rainfall, causing the Beijing area to be in a near saturated state for a long time.

3. Instability analysis
  • During the period from 0000 UTC 20 to 0600 UTC 21 July (Fig. 3) a wide range of area with an isentropic surface decreased with height, which meant the convective instability (θse/p>0) occurred over Beijing (115.5°-117.3°E). The region of strong convective instability extended to 700 hPa. At 1200 UTC 20 July (figure omitted), the isolines of pseudo-equivalent potential temperature (θ se) under 700 hPa were dense when the convective instability reached its maximum. Meanwhile, there was weak downward motion over Beijing, so no convection was triggered. At 1800 UTC 20 July (Fig. 3a), the convective instability was sustained over Beijing. It is worth noting that there was an obvious thermal inversion layer at 900 hPa, which suppressed the convection and was helpful for accumulating enough unstable energy. When the triggering condition was fulfilled, the convection occurred and torrential rain poured down. During 0600-1800 UTC 21 July the cold front moved across the Beijing area. The convective instability weakened and its height lowered. At the same time, the isentropic surfaces became oriented downward because of the latent heat released, enhancing the θ se suddenly at one place; thus, the isentropic surface became concave. At 1200 UTC 21 July (Fig. 3b) the convective instability decreased and the isentropic surface tilted to almost upright. Beijing was right at the bottom of the funnel-shaped isentropic surface. Strong upward motion occurred over Beijing, tilted westward with height. As shown in Fig. 3d, the vertical vorticity increased significantly due to the tilting of the isentropic surface (Wu et al., 1995), causing positive vorticity in the whole troposphere. The positive vorticity cooperated with divergence in the upper level and convergence in the lower level, bringing about the extreme precipitation.

    Figure 4.  (a) CAPE on the surface and wind vector (units: m s$^-1$) at 850 hPa and (b) CIN on the surface and wind vector (units: m s$^-1$) at 850 hPa, at 0000 UTC 21 July.

    Figure 3c shows the change over time of the vertical gradient of the pseudo-equivalent potential temperature and the vertical motion. From 0000 UTC 20 July a positive region occurred at 900-700 hPa, with the strongest center at 900 hPa, which was the convective instability. During 0600-1200 UTC 20 July the convective instability reached a maximum. Because there was no triggering condition active at this moment, no convection happened. From 0200 UTC 21 July the precipitation began and the convective unstable energy was released. So, the convective instability weakened and the atmosphere changed into neutral stratification. Furthermore, due to the release of latent heat the baroclinicity strengthened, causing the slantwise isentropic surface, which was favorable to formation of symmetric instability. At 0000 UTC 22 July there was convective instability again, the center of which was at 800 hPa. However, because of the corresponding downward motion, there was no convection. It can be concluded that the production of convection was premised on convective instability and then aided by dynamical triggering conditions. The precipitation did not necessarily occur during the strongest convective instability.

    Accumulating convective unstable energy in the atmosphere is one of the necessary conditions for producing strong convection. Convective available potential energy (CAPE) can represent the atmospheric buoyancy instability energy:

    \begin{equation} \label{eq1} { CAPE}=\int_{Z_{ LFC}}^{Z_{ EL}}\left(\dfrac{T_{ VP}-T_{ VE}}{T_{ VE}}\right)dz , (1)\end{equation}

    where T VP and T VE are the air parcel and environment virtual temperature, respectively. Z LFC and Z EL are the levels of free convection and balance, respectively. CAPE is the buoyancy work performed on an air parcel during the process of air rising from free height to the height of buoyancy balance, representing the intensity of unstable energy stored in the atmosphere. Furthermore, the strong convective instability needs to release unstable energy, which requires storage of sufficient unstable energy before the strong convection occurs. Convective inhibition energy (CIN) is a measure of convective inhibition quantities, representing the air parcel work performed on the environment during the rising of the air parcel from the ground (Z0) to the height of free convection (Z1):

    \begin{equation} \label{eq2} { CIN}=\int_{Z_0}^{Z_1}\left(\dfrac{T_{ VP}-T_{ VE}}{T_{ VE}}\right)d{ z} . (2)\end{equation}

    Usually, the CIN cannot be so small that the unstable energy releases piecemeal, but it also cannot be so large that it cannot produce deep convection. As shown in Fig. 4, before the precipitation (0000 UTC 21 July), high values of CAPE extended gradually from the southwest to Beijing; its maximum was located in the southwestern region of Beijing, reaching to approximately 1200 J kg-1. Because a low-level jet controlled the Beijing region, conveying the warm moist airflow with huge unstable energy to the storm continuously, it was an important reason for the maintenance and development of the convective instability. At the same time, the CIN was high, about -80 J kg-1, and it was not easy to trigger the convection. Thus, during this period of time, unstable energy accumulated for heavy rainfall. At 0600 UTC 21 July high values of CAPE covered the Beijing area, reaching a maximum of 1400 J kg-1. At this moment there was obvious moisture convergence in the lower level. The surrounding moist air continued to target the storm area, enhancing the atmospheric unstable energy (figure omitted). Meanwhile, the CIN weakened significantly, reducing to -20 J kg-1, so the convective unstable energy could be easily released without strong, dynamic lifting conditions. With the development of convection, the wind direction turned southerly; thus, the transportation of unstable energy broke off and the CAPE deceased rapidly.

  • The analysis mentioned above shows that before 0600 UTC 21 July there was convective instability in the lower level, which gradually weakened with time. In this subsection, we show how the atmosphere changed into symmetric instability after the occurrence of rainfall.

    As is well-known, symmetric instability generally refers to the instability of the air parcel during the slantwise upward performance. The MPV can be represented as:

    \begin{equation} \label{eq3} { MPV}=\dfrac{\zeta_{ a}\nabla\theta_{ se}}{\rho}=-g(\zeta+f)\dfrac{\partial\theta_{ se}}{\partial p} +g\dfrac{\partial v}{\partial p}\dfrac{\partial\theta_{ se}}{\partial x}-g\dfrac{\partial u}{\partial p}\dfrac{\partial\theta_{ se}}{\partial y} , (3)\end{equation}

    where ζ a is the absolute vorticity. θ se is pseudo-equivalent potential temperature. MPV can be divided into two portions:

    \begin{eqnarray} \label{eq4} { MPV}_1&=&-g(\zeta+f)\dfrac{\partial\theta_{ se}}{\partial p} , (4)\end{eqnarray} \begin{eqnarray} \label{eq5} { MPV}_2&=&g\dfrac{\partial v}{\partial p}\dfrac{\partial\theta_{ se}}{\partial x}- g\dfrac{\partial u}{\partial p}\dfrac{\partial\theta_{ se}}{\partial y} , (5)\end{eqnarray}

    where MPV1 is the coupling of the vertical component of absolute vorticity and the vertical gradient of the pseudo-equivalent potential temperature (θ se), which is the barotropic component. It represents the cooperation of inertial instability and convective instability. Because the absolute vorticity of large-scale motion is positive in the Northern Hemisphere, the negative or positive of MPV1 is only dependent on ∂θ se/∂p. When the atmosphere is in convective instability, ∂θ se/∂p>0 and MPV1<0. MPV2 is the baroclinic component of MPV, representing the coupling effect of moist baroclinity and the vertical shear of the horizontal wind. When MPV1>0 and MPV<0, the atmosphere is in symmetric instability.

    Figure 5 shows the change over time of MPV, MPV1 and MPV2. From 0000 UTC 20 to 0600 UTC 21 July there was negative MPV1 at a height of 900-800 hPa (Fig. 5a), signifying a convective unstable atmosphere, which was consistent with the aforementioned results. Meanwhile, MPV was also negative (Fig. 5c), signifying a symmetric unstable atmosphere. However, (Bennetts and Sharp, 1982) noted that when convective instability and symmetric instability coexist, the atmosphere is mainly dominated by convective instability because the growth rate of convective instability is larger than symmetric instability. During the period 0600-1800 UTC 21 July, due to the precipitation, the convective unstable energy was released and the atmosphere changed into neutral stratification. At this moment, MPV1≥ 0. Meanwhile, the baroclinicity and the horizontal gradient of potential temperature strengthened at 900-800 hPa due to the enhanced low-level jet and the incursion of a cold front over Beijing. Thus, MPV2 was enhanced and became negative, causing MPV<0. The condition of MPV1>0 and MPV<0 was met, so the atmosphere displayed symmetric instability during this period. In addition, it is worth noting that the strongest negative MPV2 corresponded with the maximum precipitation.

    Furthermore, based on the definition that the atmosphere is a symmetric unstable atmosphere when the slope of the isentropic surfaces is greater than the slope of the momentum, the steeper the isentropic surfaces were, the easier it was for symmetric instability to occur. Before the heavy rainfall (Fig. 3a) the isentropic surface was gentle, almost horizontally distributed. Then, at 1200 UTC 21 July (Fig. 3b) the front moved into the Beijing area, corresponding to the strongest frontal rainfall. The latent heat released redistributed the moisture and temperature, resulting in steeply inclined isentropic surfaces. This allowed the atmosphere to form the symmetric instability. Figure 6 shows the slope difference between the isentropic surface and the momentum surface over the Beijing area. There was an obvious positive region during the precipitation at 700 hPa, indicating the occurrence of the symmetric instability.

    Analysis of the convective instability and symmetric instability indicates that approximately 12-24 hours before the storm, the atmosphere was mainly in convective instability in the lower level. The convective instability experienced a weak-strong-weak process, but the heavy precipitation did not occur at the moment of strongest convective instability. With the occurrence of heavy rain, the convective instability energy was released and the convective instability weakened. At the same time, the symmetric instability was strengthened by the enhancement of atmospheric baroclinicity. The results are consistent with the conclusion of (Liu et al., 2014), who used WRF (Weather Research and Forecasting Model) simulation data to analyze the instability during precipitation.

    Figure 5.  Temporal evolution of (a) $ MPV_1$, (b) $ MPV_2$, (c) $ MPV$ (units: 10$^-5$ K m$^2$ s$^-1$ kg$^-1$) over Beijing (39.8$^\circ$-40.0$^\circ$N, 115.8$^\circ$-116.2$^\circ$E), where the black contour denotes the observation of 6-h accumulated rainfall (units: mm).

    Figure 6.  Temporal evolution of the slope difference between the isentropic surface and the momentum surface over the Beijing area, where the black contour denotes the observation of 6-h accumulated rainfall (units: mm).

4. Convective instability evolution before the rainfall
  • To explore the factors affecting the evolution of convective instability before the rainstorm and provide a theoretical basis for forecasting convective precipitation, the convective instability tendency equation was deduced.

    The thermodynamic equation in pressure coordinates is as follows:

    \begin{equation} \label{eq6} \dfrac{d\theta_{ se}}{dt}=0 . (6)\end{equation} Take the partial derivative of both sides of Eq. (7), \begin{eqnarray} \label{eq7} &&\dfrac{\partial}{\partial t}\left(\dfrac{\partial\theta_{ se}}{\partial p}\right)+ \left(\dfrac{\partial u}{\partial p}\dfrac{\partial\theta_{ se}}{\partial x}+ \dfrac{\partial v}{\partial p}\dfrac{\partial \theta_{ se}}{\partial y}+ \dfrac{\partial \omega}{\partial p}\dfrac{\partial\theta_{ se}}{\partial p}\right)+\nonumber\\ &&{v}\cdot\nabla\left(\dfrac{\partial\theta_{ se}}{\partial p}\right)=0, (7)\end{eqnarray} and substitute the mass continuity equation (∂ u/∂ x)+(∂ v/∂ y)+(?ω/∂p)=0 into Eq. (8), \begin{equation} \label{eq8} \dfrac{\partial}{\partial t}\left(\dfrac{\partial\theta_{ se}}{\partial p}\right)=-{v}\cdot\nabla\left(\dfrac{\partial\theta_{ se}}{\partial p}\right)+M , (8)\end{equation}

    where M=-(∂ u/∂p)(∂θse/∂ x)-(∂ v/∂p)(∂θse/∂ y)+ [(∂ u/∂ x)+(∂ v/∂ y)](∂θse/∂p) is the potential divergence equation (Ran et al., 2013). M represents the curl of horizontal wind rotated 90° and projected on the direction of the pseudo-equivalent potential temperature, indicating the coupling of horizontal divergence and the vertical shear of the horizontal wind. [(∂ u/∂p)(∂θse/∂ x)+ (∂ v/∂p)(∂θse/∂ y)] is the baroclinic component of M, and it also represents the vertical component of the convective vorticity vector. It reflects the coupling of vertical wind shear and atmospheric baroclinicity. [(∂ u/∂ x)+(∂ v/∂ y)](∂θse/∂p) is the barotropic component of M, representing the coupling of horizontal divergence and convective instability. -v ·▽(∂θse/∂p) is the advection of convective instability. Thus, the local variation of convective instability is mainly influenced by advection and potential divergence.

    Figure 7.  Vertical distribution of the forcing terms in Eq. (9) affecting the convective instability along 40$^\circ$N at 1200 UTC 20 July: (a) $\partial\theta_ se/\partial p$; (b) $M$; (c) $v\nabla\cdot(\partial\theta_ se)/\partial p$; (d) $-(\partial u/\partial p)(\partial\theta_ se/\partial x)-(\partial v/\partial p)(\partial\theta_ se/\partial y)$; (e) $(\partial u/\partial x+\partial v/\partial y) (\partial\theta_ se/\partial p)$ (units: 10$^-8$ K s$^-1$ m$^-1$).

    Figure 8.  Temporal evolution of the forcing terms in Eq. (9) affecting the convective instability over Beijing area (39.8$^\circ$-40.0$^\circ$N, 115.8$^\circ$-116.2$^\circ$E): (a) $\partial\theta_ se/\partial p$; (b) $M$; (c) $v\nabla\cdot(\partial\theta_ se)/\partial p$; (d) $-(\partial u/\partial p)(\partial\theta_ se/\partial x)- (\partial v/\partial p)(\partial\theta_ se/\partial y)$; (e) $(\partial u/\partial x+\partial v/\partial y)(\partial\theta_ se/\partial p)$ (units: 10$^-8$ K s$^-1$ m$^-1$).

    Figure 7 is the vertical distribution of the forcing terms in Eq. (9) affecting the convective instability at 1200 UTC 20 July. As shown in Fig. 7a, there were two unstable areas in the troposphere. One was located at 110°-114°E at 700 hPa. At this location the advection (Fig. 7c) was positive but the potential divergence (Fig. 7b) was primarily negative, so the convective instability here was mainly caused by the advection term. The other unstable area was at 116°-118°E at 900 hPa, which had a major effect on the heavy rainfall in Beijing. Analysis of the vertical distribution, the potential divergence (Fig. 7b) and the advection (Fig. 7c) indicates both had a positive area that overlapped with the convective unstable area. Thus, potential divergence and advection both played an important role in the development of convective instability. The potential divergence can be divided into barotropic and baroclinic components, as shown in Figs. 7d and e. The baroclinic termin the unstable region was negative and the barotropic term was positive, meaning that the convective instability was mainly dominated by the barotropic term, and the baroclinic term played an offsetting role.

    The temporal evolution of the forcing terms (Fig. 8) shows the convective instability from 0000 UTC 20 to 0600 UTC 21 July. Then, the convective instability weakened and the atmosphere changed into neutral stratification. Figure 8b indicates that the potential divergence was mainly positive at 900-800 hPa before the rainstorm, helping to develop and maintain the convective instability. The advection also played an important role in convective instability development, but it was relatively weaker before the rainstorm and stronger during the approaching rainfall process. Thus, the potential divergence contributed more to the convective instability. Figures 8d and e show that the barotropic component of potential divergence was primarily positive before the heavy rainfall, so it actively promoted the development of convective instability. The baroclinic component of potential divergence was weak and negative before the precipitation, having an offsetting influence. However, it gradually became stronger during precipitation, having a great impact on inhibiting the convective instability. The barotropic component of potential divergence played the most significant role in affecting the convective instability before the rainstorm. During the period of precipitation from 0000 UTC 21 to 0000 UTC 22 July the convective instability weakened, primarily due to the baroclinic component of the potential divergence mentioned above. The reason might have been that the low-level jet strengthened during the precipitation, bringing about the vertical shear of horizontal wind and the atmosphere's baroclinic enhancement. Meanwhile, the moist, warm air climbed along the cold air in front and the cold and warm airs converged, causing the slantwise isentropic surface and the horizontal gradient of pseudo-equivalent potential temperature to increase. Thus, the baroclinic component was enhanced, partially offset by the effects of the barotropic component, ultimately causing the convective instability to decrease. On the other hand, it was also an important reason for the enhancement of the symmetric instability, which can be seen in the next part.

    It can be concluded that the barotropic component of potential divergence played the leading role in promoting the development of convective instability before the rainstorm. After the storm had occurred the baroclinic term of the potential divergence suppressed the convective instability development.

5. Symmetric instability during the rainfall
  • According to the above analysis symmetric instability occurred over Beijing from 0200 UTC 21 to 1800 UTC 21 July. It reached a peak at 1200 UTC 21 July, which corresponded with the maximum precipitation.

    Further analysis is made to explore the factors affecting the evolution of symmetric instability during precipitation. Under adiabatic and frictionless conditions the potential vorticity is conservative (Wu et al., 1995):

    \begin{equation} \label{eq9} \dfrac{d{ MPV}}{dt}=0 . (9)\end{equation} Equation (10) can be rewritten as: \begin{equation} \label{eq10} \dfrac{d{ MPV}_1}{dt}+\dfrac{d{ MPV}_2}{dt}=0 . (10)\end{equation} Then, \begin{eqnarray} \label{eq11} \dfrac{d{ MPV}_2}{dt}&=&-\dfrac{d{ MPV}_1}{dt} =g\dfrac{\partial\theta_{ se}}{\partial p}\left(\dfrac{\partial\omega}{\partial y}\dfrac{\partial u}{\partial p}- \dfrac{\partial\omega}{\partial x}\dfrac{\partial v}{\partial p}\right)-\nonumber \end{eqnarray} \begin{eqnarray} &&g(\xi+f)\left(\dfrac{\partial\theta_{ se}}{\partial x}\dfrac{\partial u}{\partial p}+ \dfrac{\partial\theta_{ se}}{\partial y}\dfrac{\partial v}{\partial p}\right) ,\\[-10mm]\nonumber (11)\end{eqnarray}

    where d MPV1/dt and d MPV2/dt are the individual variations of MPV1 and MPV2, respectively. Under the premise of MPV conservation, there is a certain mutual conversion between MPV1 and MPV2. According to Eq. (10), when d MPV1/dt increases d MPV2/dt will decrease, and when d MPV1/dt decreases d MPV2/dt will increase. The conditions of MPV1>0 and MPV<0 signify symmetric instability in the atmosphere. Thus, when d MPV1/dt>0 MPV1 increases and when d MPV2/dt<0 MPV2 decreases, and the symmetric instability would be maintained and would develop. In Eq. (11), g(∂θ se/∂p)[(∂ω/∂ y)(∂ u/∂p)- (∂ω/∂ x)(∂ v/∂p)] is the coupling of the vorticity tilting term and vertical gradient of pseudo-equivalent potential temperature, and \(g(\xi +f)[(\partial\theta_ se/\partial x)(\partial u/\partial p)+ (\partial\theta_ se/\partial y)(\partial v/\partial p)]\) is the coupling of vertical vorticity and the baroclinic component of potential divergence. Thus, the individual variation of MPV2 is mainly affected by the two terms above.

    Figure 9 shows the vertical distribution of the two forcing terms of MPV2 at the moment of strongest precipitation (1200 UTC 21 July). The maximum 6-h accumulated precipitation in Beijing reached 80 mm and the gradient of each forcing term was strong in the precipitation region. The coupled term of vertical vorticity and potential divergence was relatively strong (Fig. 9b) compared with the other terms. There was a negative area at 800 hPa over Beijing, indicating d MPV2/dt decreased, thus causing MPV2 to become negative and enhancing the symmetric instability. At the same time, there was a weaker negative area to the south of the positive area. There was a wide positive zone of the first term on the right-hand side of Eq. (11) over Beijing (Fig. 9a), which was weaker than the second term, inhibiting the development of symmetric instability.

    Further analysis on the temporal evolution of the three forcing terms is shown in Fig. 10. Because there was no precipitation during the period 0000 UTC 20 to 0000 UTC 21 July, the forcing terms were all weak. From 0200 UTC 21 the heavy rain occurred in the Beijing area, and so the symmetric instability strengthened. During the precipitation, the contribution of the coupled term of vertical vorticity and potential divergence was significant (Fig. 10b). There was a strong negative area at the lower level of 900-800 hPa from 0000 UTC to 1800 UTC 21 July, corresponding to the heavy rain. The negative area caused MPV2 to decrease with time, contributing to the enhancement of symmetric instability. This term was strongest at 1200 UTC 21, corresponding to the maximum precipitation and strongest symmetric instability.The first coupled term of vorticity tilting and the vertical gradient of pseudo-equivalent potential temperature (Fig. 10a) were weak and positive, having an impact on inhibiting the development of the symmetric instability.

    Figure 9.  Vertical distribution of the forcing terms in Eq. (11) affecting the individual variation of MPV2 along 40$^\circ$N, where the black contour denotes the observation of 6-h accumulated rainfall (units: mm): (a) $g(\partial\theta_ se/\partial p)[(\partial\omega/\partial y)(\partial u/\partial p)-(\partial\omega/\partial x)$$(\partial v/\partial p)]$; (b) $-g(\xi+f)[(\partial\theta_ se/\partial x)(\partial u/\partial p)+(\partial\theta_ se/\partial y)(\partial v/$ $\partial p)]$ (units: 10$^-10$ K m$^2$ s$^-2$ kg$^-1$).

    Figure 10.  Temporal evolution of the forcing terms in Eq. (11) affecting the individual variation of MPV2 along 40$^\circ$N over the Beijing area (39.8$^\circ$-40.0$^\circ$N, 115.8$^\circ$-116.2$^\circ$E), where the black contour denotes the observation of 6-h accumulated rainfall (units: mm): (a) $g(\partial\theta_ se/\partial p)[(\partial \omega/\partial y) (\partial u/\partial p)-(\partial \omega/\partial x)$$(\partial v/\partial p)]$; (b) $-g(\xi+f)[(\partial\theta_ se/\partial x) (\partial u/\partial p)+ (\partial\theta_ se/\partial y) (\partial v/$ $\partial p)]$ (units: 10$^-10$ K m$^2$ s$^-2$ kg$^-1$).

    As seen from the analysis above, the coupling of vertical vorticity and the baroclinic component of potential divergence made the most remarkable contribution to maintaining and developing the symmetric instability during the precipitation. The reason for the anomaly of this term was the tilting of the isentropic surface due to the release of latent heat, causing rapid development of vertical vorticity. Meanwhile, the enhancement of the low-level jet increased the vertical wind shear. Moreover, a cold front moved into the Beijing area and the cold and warm air masses converged, enhancing the three-dimensional spatial gradients of the pseudo-equivalent temperature. These factors synthetically caused \(-g(\xi +f)[(\partial\theta_ se/\partial x)(\partial u/\partial p)+ (\partial\theta_ se/\partial y)(\partial v/\partial p)]\) to decrease, thus contributing to the development of symmetric instability.

    Comparing the effect of factors on convective instability and symmetric instability showed some correlation.The baroclinic component of potential divergence is the key point, which weakened the convective instability and enhanced the symmetric instability during the precipitation.

6. Conclusion
  • In this paper, using a heavy rain event that occurred in Beijing on 21 July 2012 as an example, GFS reanalysis data from NCAR-NCEP were used to analyze the characteristics and evolution mechanism of convective and symmetric instability before and during the North China rainstorm. The main conclusions can be summarized as follows:

    (1) Approximately 12 hours before the rainstorm the atmosphere was mainly dominated by convective instability in the lower level of 900-800 hPa. The strong southwesterly low-level jet conveyed the moist and warm airflow continuously to the torrential rain area, maintaining and enhancing the unstable energy. When the precipitation happened and the unstable energy was released, the convective instability weakened. Meanwhile, due to baroclinic enhancement in the atmosphere, the symmetric instability strengthened, maintaining and promoting the development of the torrential rain.

    (2) By deriving the convective instability tendency equation, the evolution characteristics and impact factors on convective instability were analyzed. Before the rainstorm the barotropic component of potential divergence and the advection of convective instability played a major role in promoting the development of convective instability. After the precipitation occurred the convective instability weakened due mainly to the baroclinic component of the potential divergence.

    (3) The primary factors affecting the development of the symmetric instability during the precipitation were the cooperation between vertical vorticity and the baroclinic component of potential divergence, as established by analyzing the MPV tendency equation. Importantly, the baroclinic component of potential divergence was the key point, which weakened the convective instability and enhanced the symmetric instability during the precipitation. When the convective instability decreased and the symmetric instability increased, the rainfall event occurred. Thus, the baroclinic component of potential divergence may be an important signal for forecasting, which needs further investigation and discussion.

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