VLF OBSERVATIONS BY THE AKEBONO (EXOS-D) SATELLITE

被引：56
作者：
KIMURA, I
HASHIMOTO, K
NAGANO, I
OKADA, T
YAMAMOTO, M
YOSHINO, T
MATSUMOTO, H
EJIRI, M
HAYASHI, K
机构：
[1] TOKYO DENKI UNIV,DEPT ELECT ENGN,TOKYO 101,JAPAN
[2] KANAZAWA UNIV,ELECT ENGN,KANAZAWA,ISHIKAWA 920,JAPAN
[3] NAGOYA UNIV,ATMOSPHER RES INST,TOYOKAWA 442,JAPAN
[4] UNIV ELECTROCOMMUN,DEPT COMMUN,CHOFU,TOKYO 182,JAPAN
[5] KYOTO UNIV,CTR RADIO ATMOSPHER SCI,UJI,KYOTO 611,JAPAN
[6] NATL INST POLAR RES,TOKYO 173,JAPAN
[7] UNIV TOKYO,GEOPHYS RES LAB,TOKYO 113,JAPAN
[8] INST SPACE & ASTRONAUT SCI,SAGAMIHARA 229,JAPAN
来源：
JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY | 1990年 / 42卷 / 04期
关键词：
D O I：
10.5636/jgg.42.459
中图分类号：
P [天文学、地球科学];
学科分类号：
07 ;
摘要：
The VLF wave instruments on board Akebono (EXOS-D) involve a wide band analyzer (WBA), multi-channel analyzers (MCA), Poynting flux analyzers, (PFX), ELF frequency analysers and vector impedance probe (VIP) and cover a frequency range from a few Hz to 17.8 kHz for electric and magnetic field components. The main objectives of the wave observations are to investigate the wave phenomena closely associated with energetic particle precipitation in the auroral zone and the physics of wave-wave and wave-particle interaction phenomena. -from Authors
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页码：459 / 478
页数：20
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