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Harmonics of whistler-mode waves near the Moon
被引:0
|作者:
Yasunori Tsugawa
Yuto Katoh
Naoki Terada
Hideo Tsunakawa
Futoshi Takahashi
Hidetoshi Shibuya
Hisayoshi Shimizu
Masaki Matsushima
机构:
[1] Tohoku University,Department of Geophysics, Graduate School of Science
[2] Tokyo Institute of Technology,Department of Earth and Planetary Sciences
[3] Kyushu University,Department of Earth and Planetary Sciences, Faculty of Science
[4] Kumamoto University,Department of Earth and Environmental Sciences
[5] University of Tokyo,Earthquake Research Institute
来源:
Earth, Planets and Space
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/
67卷
关键词:
Harmonic wave;
Nonlinear steepening;
Whistler-mode;
Solar wind;
Magnetic anomaly;
Lunar dust;
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摘要:
Harmonic spectral features of electromagnetic waves in the frequencies of several Hz around the Moon have been identified by Kaguya. The waves have steepened waveforms peculiarly in the compressional component. The fundamental waves have almost the same properties as narrowband whistler-mode waves with the frequencies near 1 Hz, which have been observed around the Moon. The waves are observed around the terminator region in the solar wind near the lunar magnetic anomalies at the altitudes under 120 km. We suggest that the harmonic spectra are a result of the nonlinear steepening of narrowband whistler-mode waves. Although the narrowband whistler-mode waves have been observed in the upstream region of many planetary bow shocks, such harmonics have rarely been observed there. Since the harmonics are more frequently observed at lower altitudes of the Moon, they are possibly caused by lunar intrinsic environments including lunar dusts and local structures of lunar magnetic anomalies.
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