Low Frequency plasma wave Analyzer (LFA) onboard the PLANET-B spacecraft

被引:0
|
作者
H. Matsumoto
T. Okada
K. Hashimoto
I. Nagano
S. Yagitani
M. Tsutsui
Y. Kasaba
K. Tsuruda
H. Hayakawa
A. Matsuoka
S. Watanabe
H. Ueda
I. Kimura
Y. Kasahara
Y. Omura
T. Matsumura
T. Imachi
K. Ishisaka
Y. Tateno
机构
[1] Kyoto University,Radio Atmospheric Science Center
[2] Toyama Prefectural University,Department of Electronics and Informatics
[3] Kanazawa University,Department of Electrical and Computer Engineering
[4] Kyoto Sangyo University,Institute for Computer Sciences
[5] Institute of Space and Astronautical Science,Department of Electrical and Electronics Engineering
[6] Communications Research Laboratory,Faculty of Information Science
[7] Chiba University,Department of Electrical Engineering II
[8] Osaka Institute of Technology,undefined
[9] Kyoto University,undefined
[10] Toshiba Information System Co. Ltd.,undefined
来源
Earth, Planets and Space | 1998年 / 50卷
关键词
Solar Wind; Plasma Wave; Ambient Plasma; Solar Wind Interaction; Wire Antenna;
D O I
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中图分类号
学科分类号
摘要
The Low Frequency plasma wave Analyzer, LFA, on board the PLANET-B spacecraft has been developed to measure the Martian plasma waves. Two orthogonal electric dipole wire antennas, 50 m tip-to-tip, in the spacecraft spin plane are used to measure plasma waves, dc electric fields, and the spacecraft potential relative to the ambient plasma. The LFA has capability to measure the wave spectrum in the band from 10 Hz to 32 kHz, and to capture the signal waveform in the band from dc to 32 kHz by using a 4 MByte memory. The LFA scientific objectives are to explore the following: (1) Macroscopic plasma environment and boundaries from the solar wind to the ionosphere, (2) Microscopic plasma phenomena induced by the interaction between the solar wind and the Martian atmosphere and the moon Phobos, (3) Generation and propagation of electromagnetic waves, (4) Plasma densities and waves in the nightside ionosphere and tail, and (5) Comparison of Martian plasma waves with those of other planets such as non-magnetized Venus and magnetized Earth.
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页码:223 / 228
页数:5
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