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Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period.
https://asahi-u.repo.nii.ac.jp/records/3419
https://asahi-u.repo.nii.ac.jp/records/34196408e081-7c7a-42ff-9c1b-53872f66c24f
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
00221392_43_685689_1991 (469.9 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2015-08-11 | |||||
| タイトル | ||||||
| タイトル | Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period. | |||||
| タイトル | ||||||
| タイトル | Quiescence of GLE-Producible Solar Proton Eruptions during the Transition Phase of Heliomagnetic Polarity Reversal near the Solar-Activity-Maximum Period. | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 資源タイプ | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
| 資源タイプ | journal article | |||||
| 著者 |
Nagashima, Kazuo
× Nagashima, Kazuo× Sakakibara, Shizuko× Morishita, Isao |
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| 所属 | ||||||
| Cosmic-Ray Section, Solar-Terrestrial Environment Laboratory, Nagoya University | ||||||
| 所属 | ||||||
| Cosmic-Ray Section, Solar-Terrestrial Environment Laboratory, Nagoya University | ||||||
| 所属 | ||||||
| Department of Information Management, Asahi University | ||||||
| 書誌情報 |
Journal of geomagnetism and geoelectricity en : Earth, Planets and Space 巻 43, 号 8, p. 685-689, 発行日 1991 |
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| 出版者 | ||||||
| Society of Geomagnetism and Earth, Planetary and Space Sciences | ||||||
| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | By using data of the ground-level-enhancement (GLE), of solar cosmic rays observed with the neutron and muon monitors in the period 1942-1990, it is shown that the solar proton eruptions producible GLE are forbidden during the transition phase of the heliomagnetic polarity reversal, near the period of the maximum solar activity. It is suggested that the quiescence of GLE is not due to the suppression effect of the proton eruption from the Sun by the strong solar magnetic field, but is due to the deterioration of the proton acceleration efficiency by the structual change of the field during the transition period. | |||||
| 内容記述 | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | By using data of the ground-level-enhancement (GLE), of solar cosmic rays observed with the neutron and muon monitors in the period 1942-1990, it is shown that the solar proton eruptions producible GLE are forbidden during the transition phase of the heliomagnetic polarity reversal, near the period of the maximum solar activity. It is suggested that the quiescence of GLE is not due to the suppression effect of the proton eruption from the Sun by the strong solar magnetic field, but is due to the deterioration of the proton acceleration efficiency by the structual change of the field during the transition period. | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 0022-1392 | |||||
| 論文ID（NAID） | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | 130003558910 | |||||
| フォーマット | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | application/pdf | |||||
| 著者版フラグ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
