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-EM13] [EE] Exploring space plasma processes with Magnetospheric Multiscale (MMS) mission

2017年5月20日(土) 10:45 〜 12:15 105 (国際会議場 1F)

コンビーナ:長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、Thomas Earle Moore(NASA Goddard Space Flight Ctr)、Benoit Lavraud(IRAP)、銭谷 誠司(自然科学研究機構国立天文台)、座長:銭谷 誠司(国立天文台)

11:15 〜 11:30

[PEM13-09] MMS衛星データを用いたEMIC波動-イオン間のエネルギー交換の直接計測

★招待講演

*北村 成寿1北原 理弘2小路 真史3三好 由純3加藤 雄人2中村 紗都子4長谷川 洋1斎藤 義文1横田 勝一郎1Giles Barbara5Moore Thomas5Gershman Daniel5,6Pollock Craig7Vinas Adolfo5Russell Christopher8Strangeway Robert8Fuselier Stephen9Burch James9 (1.宇宙航空研究開発機構 宇宙科学研究所、2.東北大学大学院 理学研究科 地球物理学専攻、3.名古屋大学 宇宙地球環境研究所、4.京都大学 生存圏研究所、5.NASA ゴダード宇宙飛行センター、6.メリーランド大学、7.Denali Scientific、8.カリフォルニア大学ロサンゼルス校 地球惑星物理学科、9.サウスウェスト研究所)

キーワード:wave particle interaction, EMIC wave, MMS spacecraft, WPIA, heavy ion, particle acceleration

Wave particle interactions, which cause particle acceleration and pitch-angle scattering, are a fundamental energy exchange process in collisionless space plasma. The four MMS (Magnetospheric Multiscale) spacecraft traversing the duskside magnetosphere measured electromagnetic ion cyclotron (EMIC) waves from ~12:18 to 12:22 UT on 1 September 2015. In this period, the burst ion data from Fast Plasma Investigation Dual Ion Spectrometer (FPI-DIS) with a time resolution of 150 ms are available. Although electric field data from probes were not usable to analyze the wave electric field due to the fluctuation with a frequency of ~0.1 Hz likely caused by ion beams from Active Spacecraft Potential Control (ASPOC) neutralizes, cold ions with energies less than 300 eV are detected by FPI-DIS due to the large magnitude of the electric field drift caused by the wave electric fields under weak background magnetic fields (~22-40 nT). Since the frequency of the EMIC waves were lower than ~1/5 of the proton gyro frequency, perpendicular electric fields were derived from the cross product of the negative cold ion velocity and the magnetic field. Using these data, we investigate energy exchange rates between EMIC waves and ions. To directly detect energy exchange between EMIC waves and energetic ions, we apply the method of Wave-Particle Interaction Analyzer (WPIA) that that is to calculate the Joule heat from dot product between the wave electric field (perpendicular component in the frequency range of 0.05-0.15 Hz in the present case) and ion resonant currents [Fukuhara et al., 2009; Katoh et al., 2013]. Near the beginning of the wave event, 15-second averages of the dot product reached -0.4 pW/m3 for ions with pitch angles of 33.25-78.75 degrees and energies of 14-30 keV. The negative value of the power in this pitch angle range indicates that the perpendicular energy of ions was being transferred to the EMIC waves propagating toward higher latitudes at the MMS location by cyclotron resonance. Ion data show non-gyrotropic distributions around the resonance velocity, and that is consistent with the nonlinear trapping of protons by the wave and formation of an electromagnetic proton hole [e.g., Omura et al., 2010]. Near the beginning of the same wave event, strongly phase bunched He+ ions up to ~2 keV with pitch angles slightly larger than 90 degrees were also detected. The dot product of the wave electric fields and He+ ion currents showed a positive value. This indicates that the He+ ions were being accelerated by the electric field of the EMIC waves. The observed feature of He+ ions is consistent with non-resonant interaction with the wave but is inconsistent with cyclotron resonance. In this event, we could measure energy transfer from hot ions to the EMIC wave and from the wave to He+ ions for the first time.