| Full text | |
| Author(s): |
Total Authors: 3
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| Affiliation: | [1] BAS, SRTI, Sofia 1113 - Bulgaria
[2] NRIAG, Cairo 11421 - Egypt
[3] Univ Sao Paulo, IAG, Inst Astron Geophys & Atmospher Sci, BR-05508090 Sao Paulo - Brazil
Total Affiliations: 3
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| Document type: | Journal article |
| Source: | SOLAR PHYSICS; v. 293, n. 2 FEB 2018. |
| Web of Science Citations: | 6 |
| Abstract | |
We present the finalized catalog of solar energetic proton events detected by the Wind/EPACT instrument over the period 1996 -2016. Onset times, peak times, peak proton intensity and onset-to-peak proton fluence are evaluated for the two available energy channels, at about 25 and 50 MeV. We describe the procedure utilized to identify the proton events and to relate them to their solar origin (in terms of flares and coronal mass ejections). The statistical relationships between the energetic protons and their origin (linear and partial correlation analysis) are reported and discussed in view of earlier findings. Finally, the different trends found in the first 8 years of Solar Cycles 23 and 24 are discussed. (AU) | |
| FAPESP's process: | 16/05254-9 - Investigating galaxy clusters in the photometric redshift space |
| Grantee: | Marcus Vinícius Costa Duarte |
| Support type: | Scholarships abroad - Research Internship - Post-doctor |