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  1. 原著論文

Solar modulation of the deep space galactic cosmic ray lineal energy spectrum measured by CRaTER, 2009-2014

https://repo.qst.go.jp/records/48228
https://repo.qst.go.jp/records/48228
fd06dd02-fa75-446e-a734-d93ac938979d
Item type 学術雑誌論文 / Journal Article(1)
公開日 2017-07-27
タイトル
タイトル Solar modulation of the deep space galactic cosmic ray lineal energy spectrum measured by CRaTER, 2009-2014
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
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 Zeitlin, Cary

× Zeitlin, Cary

WEKO 484549

Zeitlin, Cary

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W., Case A.

× W., Case A.

WEKO 484550

W., Case A.

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A., Schwadron N.

× A., Schwadron N.

WEKO 484551

A., Schwadron N.

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E., Spence H.

× E., Spence H.

WEKO 484552

E., Spence H.

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E., Mazur J.

× E., Mazur J.

WEKO 484553

E., Mazur J.

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J., Joyce C.

× J., Joyce C.

WEKO 484554

J., Joyce C.

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D., Looper M.

× D., Looper M.

WEKO 484555

D., Looper M.

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Jordan, A.

× Jordan, A.

WEKO 484556

Jordan, A.

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R., Rios R.

× R., Rios R.

WEKO 484557

R., Rios R.

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W., Townsend L.

× W., Townsend L.

WEKO 484558

W., Townsend L.

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C., Kasper J.

× C., Kasper J.

WEKO 484559

C., Kasper J.

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B., Blake J.

× B., Blake J.

WEKO 484560

B., Blake J.

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Smith, S.

× Smith, S.

WEKO 484561

Smith, S.

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Wilson, J.

× Wilson, J.

WEKO 484562

Wilson, J.

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岩田, 佳之

× 岩田, 佳之

WEKO 484563

岩田, 佳之

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Zeitlin Cary

× Zeitlin Cary

WEKO 484564

en Zeitlin Cary

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岩田 佳之

× 岩田 佳之

WEKO 484565

en 岩田 佳之

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抄録
内容記述タイプ Abstract
内容記述 The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) is an energetic particle detector flying aboard the Lunar Reconnaissance Orbiter. Since arriving at the Moon in 2009, CRaTER has observed the deep solar minimum of solar cycle 23, the ascending phase of cycle 24, the very weak maximum of cycle 24, and in recent months, what appears to be the start of the descending phase of cycle 24. In earlier work, we presented lineal energy spectra of galactic cosmic rays (GCRs) at solar minimum for different shielding depths. The long period of CRaTER observations allows us to study the evolution of these spectra as a function of solar modulation. As solar modulation increases, the total flux of GCRs decreases, and lower-energy ions are preferentially removed from the spectrum of ions that arrive in the inner heliosphere. These effects lead to modest variations in the lineal energy spectrum as a function of time. GCR fluxes at the 2009/2010 solar minimum were high by historical standards and at solar maximum remained high compared to earlier maxima.
書誌情報 Space Weather

巻 14, 号 3, p. 247-258, 発行日 2016-03
出版者
出版者 American Geophysical Union
DOI
識別子タイプ DOI
関連識別子 10.1002/2015sw001314
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