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The relationship of thermospheric density anomaly with electron temperature, small-scale FAC, and ion up-flow in the cusp region, as observed by CHAMP and DMSP satellites

机译:CHAMP和DMSP卫星观测到的热层密度异常与电子温度,小规模FAC和尖端区域离子上流的关系

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摘要

We present in a statistical study a comparison of thermospheric mass densityenhancements (ρ) with electron temperature (),small-scale field-aligned currents (SSFACs), and vertical ion velocity() at high latitudes around noon magnetic local time (MLT).Satellite data from CHAMP (CHAllenging Minisatellite Payload) and DMSP (Defense Meteorological Satellite Program) sampling the Northern Hemisphere duringthe years 2002–2005 are used. In a first step we investigate thedistribution of the measured quantities in a magnetic latitude (MLat) versusMLT frame. All considered variables exhibit prominent peak amplitudes in thecusp region. A superposed epoch analysis was performed to examine causalrelationship between the quantities. The occurrence of a thermosphericrelative mass density anomaly, ρ 1.2, in the cusp region isdefining an event. The location of the density peak is taken as a referencelatitude (Δ MLat = 0°). Interestingly, all the consideredquantities, SSFACs, , and are co-located with the densityanomaly. The amplitudes of the peaks exhibit different characters ofseasonal variation. The average relative density enhancement of the moreprominent density peaks considered in this study amounts to 1.33 during allseasons. As expected, SSFACs are largest in summer with average amplitudesequal to 2.56 μA m, decaying to 2.00 μA m in winter. The event relatedenhancements of and are both largest in winter (Δ =730 K, =136 m s) and smallest in summer (Δ = 377 K, = 57 m s. Based on the similarity of the seasonalbehaviour we suggest a close relationship between these two quantities. Acorrelation analysis supports a linear relation with a high coefficientgreater than or equal to 0.93, irrespective of season. Our preferredexplanation is that dayside reconnection fuels Joule heating of thethermosphere causing air upwelling and at the same time heating of theelectron gas that pulls up ions along affected flux tubes.
机译:我们在一项统计研究中提供了一个热电子质量密度增强(ρ)与电子温度(),小尺度场对准电流(SSFACs)和在中午磁学当地时间(MLT)附近高纬度的垂直离子速度()的比较。使用了从2002年至2005年采样的北半球CHAMP(具有挑战性的微型卫星有效载荷)和DMSP(国防气象卫星计划)的卫星数据。在第一步中,我们研究了磁纬度(MLat)与MLT框架中测量量的分布。所有考虑的变量都在尖点区域显示出明显的峰值幅度。进行了叠加时代分析,以检验数量之间的因果关系。在尖端区域发生热球相对质量密度异常ρ> 1.2定义了一个事件。密度峰的位置被视为参考纬度(ΔMLat = 0°)。有趣的是,所有考虑的数量SSFAC和与密度异常共同定位。峰值幅度表现出不同的季节变化特征。在整个季节中,本研究中考虑的最突出的密度峰的平均相对密度增加为1.33。不出所料,SSFAC在夏季最大,平均幅度等于2.56μAm,在冬季衰减至2.00μAm。和的事件相关增强在冬季(Δ= 730 K,= 136 ms)最大,而在夏季(Δ= 377 K,= 57 m s)最小。基于季节性行为的相似性,我们建议两者之间存在密切关系不管季节如何,相关分析都支持具有大于或等于0.93的高系数的线性关系,我们的优选解释是,白天的重新连接会给热球的焦耳热提供燃料,从而引起空气向上流动,同时电子气体的加热会沿离子的方向拉动离子受影响的助焊剂管。

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