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- Sakai Takasuke
- Physical Science Laboratories, College of Industrial Technologies, Nihon University
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- Kato Masahito
- Physical Science Laboratories, College of Industrial Technologies, Nihon University
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- Muraki Yasusi
- Physical Science Laboratories, College of Industrial Technologies, Nihon University
書誌事項
- タイトル別名
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- Propagation of Solar Neutron-Decay Prot
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説明
A Monte Carlo simulation of solar neutron-decay protons is performed using a simple interplanetary magnetic field (slab model) in interplanetary space. The time profile of solar neutron-decay protons obtained by our simulation is compared with observations. It is shown that the simple model can predict coherent pulses at the start of events. Magnetic field parameters used in the comparison can suggest the mean free path of protons near the Earth. The values are discussed in relation to other published results. Also, the comparisons show that it is difficult to determine the angular distribution of solar neutrons emitted at a flare site as long as the presently available solar neutron-decay protons are used.
収録刊行物
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- Ｊｏｕｒｎａｌ ｏｆ ｇｅｏｍａｇｎｅｔｉｓｍ ａｎｄ ｇｅｏｅｌｅｃｔｒｉｃｉｔｙ
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Ｊｏｕｒｎａｌ ｏｆ ｇｅｏｍａｇｎｅｔｉｓｍ ａｎｄ ｇｅｏｅｌｅｃｔｒｉｃｉｔｙ 49 (9), 1105-1113, 1997
地球電磁気・地球惑星圏学会
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詳細情報 詳細情報について
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- CRID
- 1390282681485562880
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- NII論文ID
- 130003559566
- 10002204404
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- NII書誌ID
- AA00698879
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- BIBCODE
- 1997JGG....49.1105S
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- ISSN
- 21855765
- 00221392
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- NDL書誌ID
- 4326325
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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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