日本地球惑星科学連合2023年大会

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[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM09] Space Weather and Space Climate

2023年5月25日(木) 13:45 〜 15:00 101 (幕張メッセ国際会議場)

コンビーナ:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)、Mary Aronne中村 紗都子(名古屋大学宇宙地球環境研究所)、Chairperson:Mary Aronne中村 紗都子(名古屋大学宇宙地球環境研究所)

14:30 〜 14:45

[PEM09-16] Low Energy Ion Events During Strong Storms as a Tracer of Inner Magnetosphere Dynamics

*Delores Knipp1 (1.University of Colorado Boulder)

キーワード:Low energy ions, Inner magnetosphere, Severe storms, Decadal measurements

We discuss and describe a new machine-learning-ready data set of Defense Meteorological Satellite Program (DMSP) low-energy ions. The data set covers the high activity period of solar cycle 23. These cool ions are usually present to some degree in and near the auroral zone. However, when geomagnetic activity impulsively increases these ions precipitate at low latitudes, often between 30 to 40 degrees magnetic latitudes. During severe to extreme space weather events the ions appear in the dawn longitude and then likely corotate to other local times. This unusual location for storm-time ions indicates a dynamic and complex electric field structure in the inner magnetosphere. These ions are important because they transfer energy to the ambient ionospheric electrons enhancing the sub-auroral electron temperature peak and the intensity of associated Stable Auroral Red (SAR)-arcs, potentially into the visible range. They are also a source of ion-atom auroras at mid-latitudes. The associated observations of higher energy electrons, also measured by DMSP show unusual decreases in average energy, suggesting that low-energy electrons are also enhanced at the same locations. Storm-time penetrating electric fields are possible explanations for these events. We show storm events during which these ions appear and provide scenarios for getting the low-energy ions in place. We propose that the dawn-side, low-energy ions are an additional complementary measure of storm strength (for the Dst Index) but for the inner magnetosphere.