2020年4月20日磁暴恢复相期间舌状中性结构的垂直变化

于婷婷, 任志鹏, 蔡旭光, 李韶阳. 2023. 2020年4月20日磁暴恢复相期间舌状中性结构的垂直变化. 地球物理学报, 66(11): 4437-4450, doi: 10.6038/cjg2023R0067
引用本文: 于婷婷, 任志鹏, 蔡旭光, 李韶阳. 2023. 2020年4月20日磁暴恢复相期间舌状中性结构的垂直变化. 地球物理学报, 66(11): 4437-4450, doi: 10.6038/cjg2023R0067
YU TingTing, REN ZhiPeng, CAI XuGuang, LI ShaoYang. 2023. Vertical variations of a neutral 'tongue' during the recovery phase of the geomagnetic storm on April 20, 2020. Chinese Journal of Geophysics (in Chinese), 66(11): 4437-4450, doi: 10.6038/cjg2023R0067
Citation: YU TingTing, REN ZhiPeng, CAI XuGuang, LI ShaoYang. 2023. Vertical variations of a neutral 'tongue' during the recovery phase of the geomagnetic storm on April 20, 2020. Chinese Journal of Geophysics (in Chinese), 66(11): 4437-4450, doi: 10.6038/cjg2023R0067

2020年4月20日磁暴恢复相期间舌状中性结构的垂直变化

  • 基金项目:

    国家重点研发计划(2022YFF0503901), 中国科学院B类战略重点项目(41000000), 中国科学院战略重点研究项目(XDA17010201, XDA17010404), 中国民用航空航天技术预研项目(D020105), 国家科学基金项目(41874179, 42104009, 42304178), 大型科研基础设施开放项目"基于中国子午线项目的低中纬度大气与电离层相互作用研究", 中国科学院重点部署项目(ZDRE-KT-2021-3)和中国博士后科学基金项目(2021M703192)联合资助

详细信息
    作者简介:

    于婷婷, 女, 1992年生, 中国科学院地质与地球物理研究所博士后, 目前从事热层中性成分及风场变化性研究.E-mail: ytt@mail.iggcas.ac.cn

    通讯作者: 任志鹏, 男, 1982年生, 研究员, 博士生导师, 现主要从事电离层/热层模式化和数值模拟、中低层大气-电离层/热层系统耦合等研究.E-mail: zpren@mail.iggcas.ac.cn
  • 中图分类号: P351

Vertical variations of a neutral 'tongue' during the recovery phase of the geomagnetic storm on April 20, 2020

More Information
  • 在发生于2020年4月20日的地磁暴恢复相阶段, GOLD(Global-scale Observations of the Limb and Disk)成像仪在第112天(day of year, DOY 112)中低纬地区观测到氧原子(O)和氮气分子(N2)的柱密度比(ΣO/N2)的舌状中性结构(TON).TON结构一般指发生于中高纬且形成于两个ΣO/N2暴时衰减结构之间的ΣO/N2增强结构.热层-电离层电动力学大气环流模式(Thermosphere-Ionosphere-Electrodynamics General Circulation Model, TIEGCM)定性地模拟再现了在本次磁暴恢复相期间观测到的ΣO/N2增强结构, 并且发现这个结构在前一天(DOY 111)当地下午形成, 通过中性风的输运被逐渐耗散.模拟结果呈现了不同高度O/N2的TON结构的垂直变化, 其强度和纬度范围有明显的高度依赖性, 并且随磁暴演化不断变化.诊断分析表明: 下沉流(downwelling)驱动的垂直输运首先导致较低纬(约30°N—70°N)O/N2的增强, 然后通过极向风驱动的水平输运将其向更高纬地区输运.在中低热层(约120~300 km高度), 主导O/N2的TON结构演化的中低纬极向风主要是由气压梯度力导致的, 同时科里奥利力对极向风也有一定的正贡献.而在约300 km高度以上的高热层, 极向风主要由气压梯度力和与其作用相反的垂直黏性力两项控制.

  • 加载中
  • 图 1 

    (a) AE(黑线)指数和F10.7p(蓝线)指数从2020年DOY 110到DOY 112期间的变化; (b) Dst(蓝线,蓝色虚线为Dst零值)指数和3小时Kp(黑线) 指数变化; (c) IMF By(黑线)和Bz(蓝线)变化,黑色虚线是ByBz的零值

    Figure 1. 

    (a) The variations of Auroral electrojet (AE) (black line) and F10.7p (blue line) indices from DOY 110 to DOY 112 in 2020; (b) The second panel is hourly Dst (blue line, blue dashed line is the zero value of Dst index) and the 3-h Kp (black line) and indices; (c) The By (black line) and Bz (blue line). The black dashed line is the zero value of By and Bz

    图 2 

    GOLD观测(左)和TIEGCM模拟(右)的ΣO/N2的DOY112和DOY110的暴时百分比变化在特定世界时的经纬度分布z=-1.5压力面上的水平风用黑色箭头呈现在TIEGCM模拟结果上,黑色虚线表示GOLD的观测范围.

    Figure 2. 

    Longitudinal and latitudinal distribution of the storm-quiet time percentage changes of ΣO/N2 at selected UTs between DOY 112 and 110 in GOLD observations (left) and TIEGCM simulations (right) The horizontal windson the z=-1.5 pressure level are overlaid on the panels of TIEGCM simulations. The black dotted lines indicate the GOLD FOV.

    图 3 

    北半球从DOY 111的13 UT到DOY 112的11 UT的ΣO/N2暴时百分比变化的极区图

    Figure 3. 

    Polar view of the storm-quiet time percentage changes of ΣO/N2 in the NH from TIEGCM simulations at selected UTs on DOY 111 and DOY 112

    图 4 

    从DOY 111的13 UT到18 UT TIEGCM模拟的经度为51°E的O/N2暴时百分比变化的纬度-压力面分布结果,中性风叠加在成分变化上

    Figure 4. 

    Latitude-pressure surface distributions of the storm-quiet time percentage changes in O/N2 at the longitude of 51°E from TIEGCM simulations at selected UTs on DOY 111. The neutral winds are overlaid on the panels

    图 5 

    O的总的时间变化率∂Ψo/∂t,垂直输运,水平输运,分子扩散的暴时变化在51°E处的纬度-压力面分布,对应世界时为DOY 111的14 UT,16 UT,18 UT

    Figure 5. 

    Latitude-pressure surface distributions of the storm-quiet changes in the total time rate of change of O (∂Ψo/∂t), horizontal advection, vertical advection and molecular diffusion at the longitude of 51°E from TIEGCM simulations at 14 UT, 16 UT, 18 UT on DOY 111

    图 6 

    图 5一致,对应世界时为DOY 112的2 UT,5 UT,8 UT

    Figure 6. 

    Similar to Fig. 5, but at 2 UT, 5 UT, 8 UT on DOY 112

    图 7 

    DOY 111的15.5 UT在z=-1.5(约160 km高度)压力面上ΣO/N2中暴时百分比变化,以及当天的Vn(子午风速),Vn的总时间变化率(∂Vn/∂t),科氏力,离子阻力,水平动量输运,压力梯度力和离心力的经纬度分布

    Figure 7. 

    Longitudinal and latitudinal distributionof the storm-quiet percentage changes in ΣO/N2, and the day′s Vn (meridional wind speed), the total time rate of change of Vn (∂Vn/∂t), Coriolis force, ion drag force, horizontal momentum advection, pressure gradient force and centrifugal force of Vn at 15.5 UT on DOY 111 on the z=-1.5 (~160 km) pressure surface

    图 8 

    DOY 111的15.5 UT在51°E经度ΣO/N2中暴时百分比变化,以及当天的Vn(子午风速),Vn的总时间变化率(∂Vn/∂t),垂直黏度,科里奥利力,离子阻力,水平动量平流,离心力和压力梯度力的纬度-压力面分布

    Figure 8. 

    Latitude-pressure surface distributions of the storm-quiet percentage changes in ΣO/N2, and the day′s Vn (zonal/meridional wind speed), the total time rate of change of Vn (∂Vn/∂t), vertical viscosity, Coriolis force, ion drag force, horizontal momentum advection, centrifugal force and pressure gradient force of Vn at 14 UT on DOY 111 at the longitude of 51°E

  •  

    Bruinsma S, Forbes J M, Nerem R S, et al. 2006. Thermosphere density response to the 20-21 November 2003 solar and geomagnetic storm from CHAMP and GRACE accelerometer data. Journal of Geophysical Research: Space Physics, 111(A6): A06303, doi: 10.1029/2005JA011284.

     

    Burns A G, Killeen T L, Carignan G R, et al. 1995a. Large enhancements in the O/N2 ratio in the evening sector of the winter hemisphere during geomagnetic storms. Journal of Geophysical Research: Space Physics, 100(A8): 14661-14671, doi: 10.1029/94ja03235.

     

    Burns A G, Killeen T L, Deng W, et al. 1995b. Geomagnetic storm effects in the low- to middle-latitude upper thermosphere. Journal of Geophysical Research: Space Physics, 100(A8): 14673-14691, doi: 10.1029/94ja03232.

     

    Burns A G, Wang W, Killeen T L, et al. 2004. A "tongue" of neutral composition. Journal of Atmospheric and Solar-Terrestrial Physics, 66(15-16): 1457-1468, doi: 10.1016/j.jastp.2004.04.009.

     

    Burns A G, Wang W, Killeen T L, et al. 2006. Vertical variations in the N2 mass mixing ratio during a thermospheric storm that have been simulated using a coupled magnetosphere-ionosphere-thermosphere model. Journal of Geophysical Research: Space Physics, 111(A11): A11309, doi: 10.1029/2006JA011746.

     

    Cai X G, Burns A G, Wang W B, et al. 2020. The two-dimensional evolution of thermospheric ∑O/N2 response to weak geomagnetic activity during solar-minimum observed by GOLD. Geophys. Res. Lett. , 47(18): e2020GL088838, doi: 10.1029/2020GL088838.

     

    Cai X G, Burns A G, Wang W B, et al. 2021. Investigation of a neutral "Tongue" observed by GOLD during the geomagnetic storm on May 11, 2019. Journal of Geophysical Research: Space Physics, 126(6): e2020JA028817, doi: 10.1029/2020JA028817.

     

    Cai X G, Qian L Y, Wang W B, et al. 2022a. Investigation of the post-sunset extra electron density peak poleward of the equatorial ionization anomaly southern crest. Journal of Geophysical Research: Space Physics, 127(10): e2022JA030755, doi: 10.1029/2022JA030755.

     

    Cai X G, Qian L Y, Wang W B, et al. 2022b. Hemispherically asymmetric evolution of nighttime ionospheric equatorial ionization anomaly in the American longitude sector. Journal of Geophysical Research: Space Physics, 127(11): e2022JA030706, doi: 10.1029/2022JA030706.

     

    Cai X G, Wang W B, Burns A, et al. 2022c. The effects of IMF By on the middle thermosphere during a geomagnetically "quiet" period at solar minimum. Journal of Geophysical Research: Space Physics, 127(5): e2021JA029816, doi: 10.1029/2021JA029816.

     

    Cai X G, Wang W B, Lin D, et al. 2023. Investigation of the Southern Hemisphere mid-high latitude thermospheric ∑O/N2 responses to the Space-X storm. Journal of Geophysical Research: Space Physics, 128(3): e2022JA031002, doi: 10.1029/2022JA031002.

     

    Correira J, Evans J S, Lumpe J D, et al. 2021. Thermospheric composition and solar EUV flux from the global-scale observations of the limb and disk (GOLD) mission. Journal of Geophysical Research: Space Physics, 126(12): e2021JA029517, doi: 10.1029/2021JA029517.

     

    Crowley G, Meier R R. 2008. Disturbed O/N2 ratios and their transport to middle and low latitudes. //Midlatitude Ionospheric Dynamics and Disturbances. American Geophysical Union, 181: 221-234, doi: 10.1029/181GM20.

     

    Dang T, Zhang B Z, Lei J H, et al. 2021. Azimuthal averaging-reconstruction filtering techniques for finite-difference general circulation models in spherical geometry. Geosci. Model Dev. Discuss. , 14(2): 859-873, doi: 10.5194/gmd-14-859-2021.

     

    Eastes R W, McClintock W E, Burns A G, et al. 2017. The global-scale observations of the limb and disk (GOLD) mission. Space Science Reviews, 212(1-2): 383-408, doi: 10.1007/s11214-017-0392-2.

     

    Eastes R W, McClintock W E, Burns A G, et al. 2020. Initial observations by the GOLD mission. Journal of Geophysical Research: Space Physics, 125(7): e2020JA027823, doi: 10.1029/2020JA027823.

     

    Fejer B G. 2002. Climatology and storm time dependence of nighttime thermospheric neutral winds over Millstone Hill. Journal of Geophysical Research: Space Physics, 107(A5): 1052, doi: 10.1029/2001JA000300.

     

    Foster J C, Coster A J, Erickson P J, et al. 2005. Multiradar observations of the polar tongue of ionization. Journal of Geophysical Research: Space Physics, 110(A9): A09S31, doi: 10.1029/2004JA010928.

     

    Hagan M E, Forbes J M. 2002. Migrating and nonmigrating diurnal tides in the middle and upper atmosphere excited by tropospheric latent heat release. Journal of Geophysical Research: Atmospheres, 107(D24): 4754, doi: 10.1029/2001JD001236.

     

    Hagan M E, Forbes J M. 2003. Migrating and nonmigrating semidiurnal tides in the upper atmosphere excited by tropospheric latent heat release. Journal of Geophysical Research: Space Physics, 108(A2): 1062, doi: 10.1029/2002JA009466.

     

    Klimenko M V, Zakharenkova I E, Klimenko V V, et al. 2019. Simulation and observations of the polar tongue of ionization at different heights during the 2015 St. Patrick's Day storm. Space Weather, 17(7): 1073-1089, doi: 10.1029/2018SW002143.

     

    Liu J, Wang W B, Burns A, et al. 2016. Relative importance of horizontal and vertical transports to the formation of ionospheric storm-enhanced density and polar tongue of ionization. Journal of Geophysical Research: Space Physics, 121(8): 8121-8133, doi: 10.1002/2016JA022882.

     

    Liu L B, Wan W X. 2018: Chinese ionospheric investigations in 2016—2017. Earth and Planetary Physics, (2): 89-111. doi: 10.26464/epp2018011.

     

    Mendillo M. 2006. Storms in the ionosphere: Patterns and processes for total electron content. Rev. Geophys., 44(4): RG4001, doi: 10.1029/2005RG000193.

     

    Prölss G W 2011. Density perturbations in the upper atmosphere caused by the dissipation of solar wind energy. Surv Geophys 32, 101-195. doi: 10.1007/s10712-010-9104-0

     

    Qian L Y, Burns A G, Emery B A, et al. 2014. The NCAR TIE-GCM: A community model of the coupled thermosphere/ionosphere system. //Huba J, Schunk R, Khazanov G eds. Modeling the Ionosphere-Thermosphere System. American Geophysical Union, 73-83, doi: 10.1002/9781118704417.ch7.

     

    Richmond A D, Ridley E C, Roble R G. 1992. A thermosphere/ionosphere general circulation model with coupled electrodynamics. Geophys. Res. Lett. , 19(6): 601-604. doi: 10.1029/92GL00401

     

    Roble R G, Ridley E C, Richmond A D, et al. 1988. A coupled thermosphere/ionosphere general circulation model. Geophys. Res. Lett. , 15(12): 1325-1328. doi: 10.1029/GL015i012p01325

     

    Sato T. 1959. Morphology of ionospheric F2 disturbances in the polar regions: A linkage between polar patches and plasmaspheric drainage plumes. Rep. Ionos. Space Res. Jpn. , 13: 91-95.

     

    Schunk R W, Nagy A F. 2000. Ionospheres: Physics, Plasma Physics and Chemistry. Cambridge: Cambridge University Press.

     

    Strickland D J, Evans J S, Paxton L J. 1995. Satellite remote sensing of thermospheric O/N2 and solar EUV. 1. Theory. J Geophys. Res. : Space Phys. , 100(A7): 12217-12226. doi: 10.1029/95JA00574

     

    Wang W B, Burns A G, Wiltberger M, et al. 2008. Altitude variations of the horizontal thermospheric winds during geomagnetic storms. Journal of Geophysics Research: Space Physics, 113(A2): A02301, doi: 10.1029/2007JA012374.

     

    Weimer D R. 2005. Improved ionospheric electrodynamic models and application to calculating joule heating rates. Journal of Geophysical Research: Space Physics, 110(A5): A05306, doi: 10.1029/2004JA010884.

     

    Yizengaw E, Moldwin M B, Komjathy A, et al. 2006. Unusual topside ionospheric density response to the November 2003 superstorm. Journal of Geophysical Research: Space Physics, 111(A2): A02308, doi: 10.1029/2005JA011433.

     

    Yu T T, Wang W B, Ren Z P, et al. 2021a. Middle-Low latitude neutral composition and temperature responses to the 20 and 21 November 2003 superstorm from GUVI dayside limb measurements. Journal of Geophysical Research: Space Physics, 126(8): e2020JA028427, doi: 10.1029/2020ja028427.

     

    Yu T T, Wang W B, Ren Z P, et al. 2021b. The response of middle thermosphere (~160 km) composition to the November 20 and 21, 2003 superstorm. Journal of Geophysical Research: Space Physics, 126(10): e2021JA029449, doi: 10.1029/2021ja029449.

     

    Yu T T, Cai X G, Ren Z P, et al. 2022a. Investigation of the ΣO/N2 depletion with latitudinally tilted equatorward boundary observed by GOLD during the geomagnetic storm on April 20, 2020. Journal of Geophysical Research: Space Physics, 127(12): e2022JA030889, doi: 10.1029/2022JA030889.

     

    Yu T T, Wang W B, Ren Z P, et al. 2022b. Diagnostic analysis of the physical processes underlying the long-duration ΣO/N2 depletion during the recovery phase of the 8 June 2019 geomagnetic storm. Journal of Geophysical Research: Space Physics, 127(12): e2022JA031075, doi: 10.1029/2022JA031075.

     

    Zhai C Z, Cai X G, Wang W B, et al. 2023. Mid-latitude ionospheric response to a weak geomagnetic activity event during solar minimum. Journal of Geophysical Research: Space Physics, 128(1): e2022JA030908, doi: 10.1029/2022JA030908.

     

    Zhang S R, Erickson P J, Foster J C, et al. 2015. Thermospheric poleward wind surge at midlatitudes during great storm intervals. Geophys. Res. Lett. , 42(13): 5132-5140, doi: 10.1002/2015GL064836.

     

    Zhang Y, Paxton L J, Kil H, et al. 2003. Negative ionospheric storms seen by the IMAGE FUV instrument. Journal of Geophysical Research: Space Physics, 108(A9): 1343, doi: 10.1029/2002JA009797.

     

    Zhang Y, Paxton L J, Morrison D, et al. 2004. O/N2 changes during 1-4 October 2002 storms: IMAGE SI-13 and TIMED/GUVI observations. Journal of Geophysical Research: Space Physics, 109(A10): A10308, doi: 10.1029/2004JA010441.

  • 加载中

(8)

计量
  • 文章访问数: 
  • PDF下载数: 
  • 施引文献:  0
出版历程
收稿日期:  2023-02-06
修回日期:  2023-05-16
上线日期:  2023-11-10

目录