JpGU-AGU Joint Meeting 2017

講演情報

[EE] 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-EM16] [EE] Physics of Inner Magnetosphere Coupling

2017年5月23日(火) 15:30 〜 17:00 A02 (東京ベイ幕張ホール)

コンビーナ:Danny Summers(Memorial University of Newfoundland)、Jichun Zhang(University of New Hampshire Main Campus)、海老原 祐輔(京都大学生存圏研究所)、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)、Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory)、Dae-Young Lee(Chungbuk Natl Univ)、Yiqun Yu(Beihang University)、三好 由純(名古屋大学宇宙地球環境研究所)、座長:Ukhorskiy Aleksandr(Johns Hopkins University Applied Physics Laboratory)

15:45 〜 16:00

[PEM16-14] Occurrence of EMIC waves and plasmaspheric plasmas derived from THEMIS
observations in the outer magnetosphere

★招待講演

*Khan-Hyuk Kim1Gi-Jeong Kim1Dong-Hun Lee1 (1.School of Space Research, Kyung Hee University)

キーワード:EMIC waves, Plasmaspheric plasma

We have statistically studied the relationship between electromagnetic ion cyclotron (EMIC)
waves and cold plasmaspheric plasma (Nsp) in the L range of 6-12 using the Time History of
Events and Macroscale Interactions during Substorms (THEMIS) data for 2008-2011. The
important observational results are as follows: (1) Under quiet geomagnetic conditions (Kp =
0-1), the maximum occurrence rate of the hydrogen (H) band EMIC waves appears in the early
morning sector (0600-0900 MLT) at the outermost region (L = 10-12). (2) Under moderate and
disturbed conditions (Kp > 2), the H-band occurrence rate is higher in the morning-to-early
afternoon sector for L > 10. (3) The high occurrence region of helium (He) band waves for Kp =
0-1 varies from L = 7 to 12 in radial distances along the local time (i.e., at L ~ 7 near noon and
at L = 8-12 near late afternoon). (4) The He-band waves for Kp > 2 are mainly localized
between 1200 and 1800 MLT with a peak around 1500-1600 MLT at L = 8-10. (5) Nsp is much
higher for the He-band intervals than for the H-band intervals by a factor of 10 or more. The He-band
high occurrence appears at a steep Nsp gradient region. (6) The morning-afternoon
asymmetry of the normalized frequency seen both in H and He bands is similar to the
asymmetric distribution of Nsp along the local time. These observations indicate that the cold
plasma density plays a significant role in determining the spectral properties of EMIC waves.
We discuss whether a morning-afternoon asymmetry of the EMIC wave properties can be
explained by the spatial distribution of cold plasmaspheric plasma.