Local time dependence of the frequency of Pi2 waves simultaneously observed at 5 low-latitude stations
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- Han Desheng
- Department of Geophysics, Graduate School of Science, Kyoto University
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- Iyemori Toshihiko
- Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University
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- Gao Yufen
- Institute of Geophysics, CSB
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- Sano Yasuharu
- Department of Information Management, School of Business Administration, Asahi University
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- Yang Fuxi
- Urumqi Basic Seismic Station Urumqi
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- Li Wansheng
- Yinchuan Geomagnetic Observatory
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- Nosé Masahito
- Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University
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説明
One-second resolution geomagnetic data from 5 stations located at low-latitudes (i.e., L = 1.2-1.6) were used to examine the local time dependence of the dominant frequency of Pi2 pulsations. We analyzed 183 Pi2 events simultaneously recorded at the 5 stations and discussed their possible generation mechanisms. The averaged dominant frequency of the H (horizontal) component is higher on the dawn side than that on the dusk side and shows a peak value in the post-midnight at around 03 LT, which confirms the LT dependence previously suggested from single station data (i.e., non-simultaneous observation). However, some of the events have no LT dependence. For the events which show the LT dependence at low-latitudes, we infer that the cavity resonance mode is a plausible generation mechanism, but we do not rule out the possibility of the plasmaspheric surface wave mode which has also been suggested. For the events having a common frequency between the eastern and western stations, we suggest the cavity resonance mode to be the mechanism. The averaged dominant frequency of the D component does not show any clear LT dependence, and only about 20% of Pi2s have identical frequency for both the H and D components, therefore we suggest that the H and D oscillations of Pi2s are generated from different mechanisms. We also found that the frequency of different parts of a Pi2 pulsation, i.e., the dominant frequency for leading part and trailing part of the pulsation, is different, and the frequency of the trailing part is lower than that of the leading part.
収録刊行物
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- Earth, Planets and Space
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Earth, Planets and Space 55 (10), 601-612, 2003
地球電磁気・地球惑星圏学会 、公益社団法人 日本地震学会、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会
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詳細情報 詳細情報について
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- CRID
- 1390001206512329856
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- NII論文ID
- 10011943680
- 130003780940
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- NII書誌ID
- AA11211921
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- ISSN
- 18805981
- 13438832
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- NDL書誌ID
- 6794627
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- NDL
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