日本地球惑星科学連合2021年大会

講演情報

[E] ポスター発表

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-EM11] Coupling Processes in the Atmosphere-Ionosphere System

2021年6月4日(金) 17:15 〜 18:30 Ch.04

コンビーナ:Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、Chang Loren(Institute of Space Science, National Central University)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Yue Deng(University of Texas at Arlington)

17:15 〜 18:30

[PEM11-P17] Effects of static electric fields and Alfvén waves on Joule heating in the cusp

*大井川 智一1、品川 裕之2、田口 聡1 (1.京都大学大学院理学研究科地球惑星科学専攻地球物理学教室、2.国立研究開発法人情報通信研究機構)

キーワード:質量密度異常、カスプ、ジュール加熱、アルヴェン波、電離層アルヴェン共鳴、数値モデル

Remarkable enhancements of the thermospheric mass density around the 400-km altitude in the cusp region have been observed by the CHAllenging Minisatellite Payload (CHAMP) satellite. Many modeling studies have been conducted to reproduce the mass density anomaly. Under geomagnetically disturbed conditions, previous studies have partially been successful in reproducing the mass density anomaly, while still facing difficulties in reproducing sufficient mass density enhancements under quiet conditions. In this study, we first employed a high-resolution two-dimensional local model to gain insights into what extent the static electric field and electron precipitation can explain the mass density enhancements. We found that the calculated mass density enhancement is 10% at most, which is significantly smaller than the observations by the CHAMP satellite (33% on average). The results also showed that the neutral-ion drag process suppresses Joule heating and neutral mass density enhancements, as well as the chemical reaction process. In contrast to the previous modeling studies, the model calculation imposing only the static electric field and electron precipitation cannot explain the mass density anomaly. The discrepancy between our modeling result and the satellite observation suggests the existence of additional energy sources. Recent studies have reported that electric field variability by Alfvén waves can play an important role in the neutral response in the auroral region. Alfvén waves are reflected between the E layer and the sharp slope of the Alfvén velocity above the F layer, and some are finally absorbed. This process is known as the ionospheric Alfvén resonator (IAR). Joule heating rates generated by Alfvén waves are maximized at F layer altitudes, with the altitude profile depending on wavelength and frequency. In contrast, static electric fields maximize Joule heating rates at E layer altitudes. In this study, we include Alfvén waves in our numerical model, and the impacts on Joule heating are evaluated. We will report the effects of both static electric fields and Alfvén waves on Joule heating using model calculations.