首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Dependence of thermospheric zonal winds on solar flux, geomagnetic activity, and hemisphere as measured by CHAMP
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Dependence of thermospheric zonal winds on solar flux, geomagnetic activity, and hemisphere as measured by CHAMP

机译:热散对风对冠军衡量的太阳能通量,地磁活动和半球的依赖性

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摘要

The thermospheric zonal winds measured by the CHAllenging Minisatellite Payload (CHAMP) satellite are used to statistically determine the climatology under quiet and active geomagnetic conditions. By collectively analyzing the bin-averaged wind trend with F_(10.7) and the solar-induced difference in wind structures, the solar flux dependence of global thermosphere zonal wind is determined. The increase of solar flux enhances the eastward winds at low latitudes from dusk to midnight. The increased ion drag reduces the nighttime eastward wind in the subauroral latitudes, and the daytime westward winds from 06 to 08 MLT at all latitudes decrease with increasing solar flux. Zonal winds show coupled seasonal/extreme ultraviolet (EUV) dependency. The equatorial zonal winds from 18 to 04 magnetic local time (MLT) indicate weaker eastward winds during the June solstice at high solar flux levels. Quiet time eastward winds at subauroral latitudes from 16 to 20 MLT are further decreased in the winter hemisphere. Influenced by asymmetries in solar illumination and the magnetic field, zonal winds show hemispheric asymmetries. Quiet daytime winds are additionally influenced by solar illumination effects, and the westward winds at the middle and subauroral latitudes are always stronger in the summer. The nighttime eastward winds are higher in the winter hemisphere during the solstices, as in the Southern Hemisphere during equinoxes, with the winter-summer asymmetry lessened or receding at the solar maxima. Storm-induced subauroral westward disturbancewinds are higher in the summer hemisphere and in the Northern Hemisphere during equinoxes. At a high level of solar flux, the westward disturbance winds are comparable in the two hemispheres during December solstice. Geomagnetic disturbance wind observations from CHAMP agree well with the empirical geomagnetic disturbance wind model, except for stronger subauroral westward jets. Westward winds during the afternoon may be enhanced in t
机译:通过具有挑战性的小型卫星有效载荷(CHAMP)卫星测量的热散门风用于在安静和积极的地磁条件下统计地确定气候学。通过集体分析与F_(10.7)和风力结构的太阳能触发差异,确定了全球热圈危险风的太阳能通量依赖性。太阳能的增加从黄昏到午夜的低纬度地增强了向东风。增加的离子阻力会减少亚前列潜水中的夜间向东风,随着太阳能通量的增加,06到08 MLT的日间向西风从06到08 MLT减少。 Zonal Winds显示耦合季节性/极端紫外线(EUV)依赖性。从18至04磁性局部时间(MLT)的赤道Zonal风在6月在高太阳能通量水平下的六月溶液期间表示较弱的东西。冬季半球,亚前列腺灭绝的安静时间向东潜伏的潜水进一步降低。在太阳能照射和磁场中受不对称的影响,Zonal Winds显示出半球的不对称。安静的日间风也受到太阳能照明效果的影响,中间和亚撒列的向西风在夏天总是更强大。冬季半球的夜间向东风在斯托克斯期间的冬季半球在昼夜昼夜南半球,冬季夏季不对称在太阳能最大值上减少或后退。夏季半球和北半球在昼夜昼夜北半球的偏离偏离的亚尾西方扰动。在高水平的太阳能通量下,西方干扰风在12月溶剂期间的两个半球上可比较。冠军的地磁干扰风观与经验性地磁干扰风模型相得益彰,除了亚前养牛网喷气式飞机更强。下午的西风可能会在t中加强

著录项

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  • 作者单位

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 空间物理;
  • 关键词

    Dependence; thermospheric; zonal;

    机译:依赖性;热散;纬向;

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