抄録
The measurement of the directional distribution of incident particles was made by using the Real time Radiation Monitoring Device (RRMD)-III placed inside the Space Shuttle STS-84 cruised at an altitude of 400 km and an inclination angle of 51.6°, which are the same as the cruising orbit of the International Space Station (ISS). The directional distributions of incident particles were evaluated over the observed linear energy transfer (LET) range (1-100 keV/μm). The pitch angle distribution is also obtained using the geomagnetic model of IGRF-95. The result is roughly in good agreement with the distribution obtained by the VF1-MIN anisotropy model calculation within the present experimental errors, if the shielding distribution is assumed to be uniform.
本文言語 | English |
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論文番号 | 1999JA900231 |
ページ(範囲) | 22793-22799 |
ページ数 | 7 |
ジャーナル | Journal of Geophysical Research: Space Physics |
巻 | 104 |
号 | A10 |
出版ステータス | Published - 1999 |
ASJC Scopus subject areas
- 地球化学および岩石学
- 地球物理学
- 地球惑星科学(その他)
- 宇宙惑星科学
- 大気科学
- 天文学と天体物理学
- 海洋学