JpGU-AGU Joint Meeting 2017

講演情報

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

2017年5月24日(水) 13:45 〜 15:15 ポスター会場 (国際展示場 7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)

[PEM16-P01] Software-type Wave-Particle Interaction Analyzer on board the ARASE satellite

*小嶋 浩嗣1加藤 雄人2疋島 充3高島 健3浅村 和史3三好 由純4笠原 禎也5笠原 慧6三谷 烈史3東尾 奈々7松岡 彩子3篠原 育3 (1.京都大学生存圏研究所、2.東北大学大学院理学研究科、3.宇宙航空研究開発機構宇宙科学研究所、4.名古屋大学宇宙地球環境研究所、5.金沢大学総合メディア基盤センター、6.東京大学大学院理学研究科、7.宇宙航空研究開発機構研究開発部門)

The Wave-particle interaction analyzer (WPIA) is a new method of observing wave-particle interactions in space. Based on the cutting-edge of technologies in the onboard instruments, the Software-type WPIA (S-WPIA) is installed in the ARASE satellite, which was successfully launched on December 20, 2016. The present paper introduces the principles of the WPIA and describes the detailed design of the S-WPIA on board the ARASE satellite. Understanding wave-particle interactions is essential in the study on space plasma environments, because space plasmas are collisionless and their kinetic energies are transferred through wave-particle interactions. In the conventional way of the study on wave-particle interactions via satellites, we have compared features of plasma waves with velocity distribution functions. However, that conventional way is not appropriate for identifying wave-particle interactions quantitatively. The nature of wave-particle interactions lies in the phase difference between electric field vectors(E) and velocity vectors of particles(V). This appears as the inner product form as EV. The conventional way using velocity distribution functions misses the information of this phase difference, because the velocity distribution function is obtained on the time integration basis. The WPIA overcomes the above problem in the conventional method by handling each detected particle and instant electric field intensity with keeping the enough accuracy in the relative time difference between them. The ARASE satellite and its onboard S-WPIA instrument should be frontiers in the study of wave-particle interactions. The leading edge of the system in the ARASE satellite allows us to collect whole information of particles at every particle detection timing and instant electric fields at every sampling timing. The collected particle and waveform data are stored on the onboard data storage called Mission Data Recorder (MDR). The S-WPIA calculates the phase difference and other quantities onboard reading out the data from the MDR and send the results as well as raw data of particles and plasma waves to the ground.
The main objective of the S-WPIA on board the ARASE satellite is to detect quantitatively the wave-particle interaction related to the generation of the Chorus emissions. The SWPIA also targets the quantitative detection of accelerations of electrons due to plasma waves. The function of the S-WPIA has been already confirmed during the initial operation of the ARASE satellite. The present paper introduces the details of the S-WPIA and discuss the strategy how we meet the objective of the S-WPIA in the operation.