日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

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-EM13] Dynamics of the Inner Magnetospheric System

2023年5月23日(火) 09:00 〜 10:30 オンラインポスターZoom会場 (1) (オンラインポスター)

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、三好 由純(名古屋大学宇宙地球環境研究所)、Theodore E Sarris(Democritus University of Thrace)、Evan G Thomas(Dartmouth College)

現地ポスター発表開催日時 (2023/5/23 17:15-18:45)

09:00 〜 10:30

[PEM13-P26] Ducted propagations of whistler mode waves in density enhanced and depression ducts observed by the Arase satellite

安福 友梨1、*土屋 史紀1栗田 怜2笠羽 康正1加藤 雄人1吹澤 瑞貴3笠原 禎也6松田 昇也6熊本 篤志1北原 理弘1三好 由純1中村 紗都子4松岡 彩子7篠原 育5 (1.東北大学、2.京都大学生存圏研究所、3.国立極地研究所、4.名古屋大学宇宙地球環境研究所、5.宇宙科学研究所、6.金沢大学、7.京都大学)

キーワード:ホイッスラモード波、放射線帯

Ducted propagation of whistler mode waves in the magnetosphere is of great importance for the generation of microbursts and resultant loss of radiation belt electrons. Theoretical and simulation studies have shown the propagation characteristics of ducting of whistler mode waves, and in-situ satellite observations have reported many cases that suggest ducting based on the correlation between changes in electron density and changes in wave intensity. To the best of our knowledge, there is only one quantitative comparison between observations of ducting whistler and the ducting theory: a report on the duct propagation of a whistler-mode chorus along high-density ducts (HDDs) (Chen et al., 2021).
Here, we report on the following four modes of ducted propagation cases of whistler mode waves along the increase/decrease of electron density observed by the Arase satellite. (1) Lower-Band (LB) waves propagating along the HDD with wave normal angle (WNA) of around 0 deg, (2) LB waves propagating along the low density duct (LDD) with WNAs distributed between 0 deg and over Gendrin angle, (3) LB waves propagating along the LDD
with WNAs of around Gendrin angle, (4) Upper-band waves propagating along the LDD with WNA of around 0 deg. We estimated the WNAs for each case using singular value decomposition (SVD) method (Santolík et al., 2003) and their characteristics were consistent with ducting theory (Smith et al., 1960). We calculated the frequency range in which waves are ducted based on the ducting theory. We compared this frequency range with the intensity of the observed whistler mode waves and found that the observations were consistent with the theoretical prediction. Furthermore, it is suggested that the WNAs for the cases (2) and (3) have azimuthal distributions based on the comparison between the observations and the SVD analysis of the simulated waveforms.