MHD wave characteristics inferred from correlations between X-rays, VLF, and ULFs at Syowa Station, Antarctica and Tjornes, Iceland (L~6)
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- Hirasima Yo
- Department of Physics, Rikkyo University
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- Shimobayashi Hisashi
- Department of Physics, Rikkyo University
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- Yamagishi Hisao
- National Institute of Polar Research
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- Suzuki Hiromu
- Department of Physics, Rikkyo University
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- Murakami Hiroyuki
- Department of Physics, Rikkyo University
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- Yamada Akihiro
- Department of Physics, Rikkyo University
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- Yamagami Takamasa
- The Institute of Space and Astronautical Science
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- Namiki Michiyoshi
- The Institute of Space and Astronautical Science
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- Kodama Masahiro
- The Institute of Physical and Chemical Research
書誌事項
- タイトル別名
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- MHD wave characteristics inferred from correlations between X-rays, VLF, and ULFs at Syowa Station, Antarctica and Tjörnes, Iceland (L - 6)
- MHD wave characteristics inferred from correlations between X-rays, VLF, and ULFs at Syowa Station, Antarctica and Tjörnes, Iceland (L∼6)
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The Polar Patrol Balloon No. 6 (PPB#6) observed quasi-periodic pulsations of bremsstrahlung X-rays (E = 30 - 120 keV) in the daytime of 0855 UT (0914 MLT) - 1630 UT (1614 MLT) on January 5, 1993, near Syowa Station, Antarctica (L - 6). The X-ray pulsations near the noon (1208 : 00 UT (1216 MLT) - 1225 : 04 UT (1232 MLT) ) include a period of about 260 sec, which corresponds to Pc 5 magnetic pulsations. It was found that at Syowa Station and Tjörnes, Iceland, which are both pair locations of the geomagnetic conjugacy, the X-ray pulsations are in correlation with the ULF-D pulsations. Also the Tjörnes VLF (2 kHz) pulsations correlated well with the X-ray pulsations of the period corresponding to Pc 5. It is probable that the VLF- and ULF-associated X-rays or precipitating energetic electrons in the vicinity of the L - 6 shell are in synchronization with the electron-cyclotron resonance. Lastly, the so-called ballooning-mirror instability (the BMI) is a candidate to explain the compressional MHD waves that occur during the short time interval (1216 MLT - 1232 MLT) in which the experimental results were interpreted.
収録刊行物
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- Earth, Planets and Space
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Earth, Planets and Space 51 (1), 33-41, 1999
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
- 1390001206510960128
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- NII論文ID
- 10003737040
- 130003955937
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- NII書誌ID
- AA11211921
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- ISSN
- 18805981
- 13438832
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- NDL書誌ID
- 4657946
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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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