Charge-Sign Dependent Cosmic-Ray Modulation Observed with the Calorimetric Electron Telescope on the International Space Station
書誌事項
- 公開日
- 2023-05-25
- 資源種別
- journal article
- 権利情報
-
- https://creativecommons.org/licenses/by/4.0/
- DOI
-
- 10.1103/physrevlett.130.211001
- 10.48550/arxiv.2305.16655
- 公開者
- American Physical Society (APS)
この論文をさがす
説明
We present the observation of a charge-sign dependent solar modulation of galactic cosmic rays (GCRs) with the CALorimetric Electron Telescope onboard the International Space Station over 6 yr, corresponding to the positive polarity of the solar magnetic field. The observed variation of proton count rate is consistent with the neutron monitor count rate, validating our methods for determining the proton count rate. It is observed by the CALorimetric Electron Telescope that both GCR electron and proton count rates at the same average rigidity vary in anticorrelation with the tilt angle of the heliospheric current sheet, while the amplitude of the variation is significantly larger in the electron count rate than in the proton count rate. We show that this observed charge-sign dependence is reproduced by a numerical ``drift model'' of the GCR transport in the heliosphere. This is a clear signature of the drift effect on the long-term solar modulation observed with a single detector.
main text: 6 pages, 3 figures, supplemental material: 8 pages, 3 figures, 1 table
収録刊行物
-
- Physical Review Letters
-
Physical Review Letters 130 (21), 211001-, 2023-05-25
American Physical Society (APS)
- Tweet
キーワード
詳細情報 詳細情報について
-
- CRID
- 1360021390747497984
-
- ISSN
- 10797114
- 00319007
-
- HANDLE
- 11365/1241418
- 2158/1331053
-
- PubMed
- 37739390
-
- 資料種別
- journal article
-
- データソース種別
-
- Crossref
- KAKEN
- OpenAIRE
