Software-type Wave–Particle Interaction Analyzer on board the Arase satellite

Earth, Planets and Space - Tập 70 - Trang 1-9 - 2018
Yuto Katoh1, Hirotsugu Kojima2, Mitsuru Hikishima3, Takeshi Takashima3, Kazushi Asamura3, Yoshizumi Miyoshi4, Yoshiya Kasahara5, Satoshi Kasahara6, Takefumi Mitani3, Nana Higashio7, Ayako Matsuoka3, Mitsunori Ozaki5, Satoshi Yagitani5, Shoichiro Yokota8, Shoya Matsuda4, Masahiro Kitahara1, Iku Shinohara3
1Department of Geophysics, Graduate School of Science, Tohoku University, Sendai, Japan
2Research Institute for Sustainable Humanosphere, Kyoto University, Gokasho, Uji, Japan
3ISAS/JAXA, Sagamihara, Japan
4Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan
5Graduate School of Natural Science and Technology, Kanazawa University, Kakuma, Japan
6Graduate School of Science, The University of Tokyo, Bunkyo-ku, Japan
7RDD, JAXA, Tsukuba, Japan
8Osaka University, Toyonaka, Japan

Tóm tắt

We describe the principles of the Wave–Particle Interaction Analyzer (WPIA) and the implementation of the Software-type WPIA (S-WPIA) on the Arase satellite. The WPIA is a new type of instrument for the direct and quantitative measurement of wave–particle interactions. The S-WPIA is installed on the Arase satellite as a software function running on the mission data processor. The S-WPIA on board the Arase satellite uses an electromagnetic field waveform that is measured by the waveform capture receiver of the plasma wave experiment (PWE), and the velocity vectors of electrons detected by the medium-energy particle experiment–electron analyzer (MEP-e), the high-energy electron experiment (HEP), and the extremely high-energy electron experiment (XEP). The prime objective of the S-WPIA is to measure the energy exchange between whistler-mode chorus emissions and energetic electrons in the inner magnetosphere. It is essential for the S-WPIA to synchronize instruments to a relative time accuracy better than the time period of the plasma wave oscillations. Since the typical frequency of chorus emissions in the inner magnetosphere is a few kHz, a relative time accuracy of better than 10 μs is required in order to measure the relative phase angle between the wave and velocity vectors. In the Arase satellite, a dedicated system has been developed to realize the time resolution required for inter-instrument communication. Here, both the time index distributed over all instruments through the satellite system and an S-WPIA clock signal are used, that are distributed from the PWE to the MEP-e, HEP, and XEP through a direct line, for the synchronization of instruments within a relative time accuracy of a few μs. We also estimate the number of particles required to obtain statistically significant results with the S-WPIA and the expected accumulation time by referring to the specifications of the MEP-e and assuming a count rate for each detector.

Tài liệu tham khảo

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