首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Impact of 10 January 1997 geomagnetic storm on the nighttime Weddell Sea Anomaly: A study utilizing data provided by the TOPEX/Poseidon mission and the Defense Meteorological Satellite Program, and simulations generated by the Coupled Thermosphere/Io
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Impact of 10 January 1997 geomagnetic storm on the nighttime Weddell Sea Anomaly: A study utilizing data provided by the TOPEX/Poseidon mission and the Defense Meteorological Satellite Program, and simulations generated by the Coupled Thermosphere/Io

机译:1997年1月10日地磁风暴的影响夜间威德尔海异常:一项研究利用TOPEX /波塞冬任务和提供的数据国防气象卫星计划模拟生成的耦合热电离层/ Io

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This study investigates the evolution of 10 January 1997 magnetic storm and the nighttime space weather change created by the impact of the interplanetary shock wave and associated events on the ionosphere. Its aims are to trace the storm's energy flow dissipation and transportation processes and to learn about the response of nighttime ionosphere to these interplanetary events, focusing on the reaction of the nighttime Weddell Sea Anomaly (WSA). To track down the consequential space weather changes, multi-instrument measurements and Coupled Thermosphere/Ionosphere Plasmasphere (CTIP) simulations were combined. As results show, the first response of nighttime WSA to the energy input in the magnetosphere, when BZ turned southward, was its ~50% total electron content (TEC) and Ni increase maintained during the main phase, indicating long-duration positive storm effects. At ~0800 universal time (UT) the second such BZ event triggered the depletion of equatorial and northern midlatitude ionosphere, a signature of strong downward E × B plasma drift, and launched gravity waves. Following a period of very bright aurora, at ~1200 UT, some southern midlatitude and subauroral plasma enhancements developed. TOPEX detected an enhancement between 45–65°S (dip), where the equatorward winds were most effective, with a sudden TEC drop-off, a signature of the plasmapause. Particularly strong negative storm effects depleted the nighttime WSA's TEC-Ni (~45–50%) and O/N2 ratio (~21%). The Bent model could simulate the WSA, but not the storm-related ionospheric responses. CTIP simulations indicated equatorward winds causing downwellings and changes in the neutral atmospheric composition revealed by the O/N2 ratio. Joule heating and electric fields were the major geophysical factors observed changing space weather during this storm.
机译:本研究调查10的进化1997年1月磁暴和夜间空间天气的变化产生的影响行星际激波和相关事件在电离层。风暴的能量耗散和流动运输流程和了解回应的夜间电离层星际事件,关注反应夜间的威德尔海异常(WSA)。跟踪天气的重要空间变化,multi-instrument测量和耦合热大气层电离层等离子体层(CTIP)模拟的总和。显示,夜间WSA的第一反应在磁层能量输入,当热晕向南,是它~ 50%总电子含量(TEC)和镍在主要增加维护阶段,表明长期积极的风暴效果。这样商务事件引起的损耗赤道和北部中间纬度电离层签名的强劲向下E×B等离子体漂移,,并推出了重力波。非常明亮的极光,~ 1200 UT,一些南部中间纬度和subauroral等离子体增强发展。45 - 65°S(下降),朝赤道方向的风突然TEC下降,最有效的等离子体层顶的签名。消极的减少夜间风暴影响WSA TEC-Ni(~ 45 - 50%)和O / N2比率(~ 21%)。弯曲的模型可以模拟WSA,但不是马萨诸塞州电离层响应。模拟显示朝赤道方向风造成的下降和中性的变化大气成分显示O / N2比率。主要地球物理因素观察变化的空间天气在这风暴。

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