Energy Dependence of Solar Energetic Protons and Their Origin in Solar Cycles 23 and 24-Reference-Cited by-同舟云学术

Energy Dependence of Solar Energetic Protons and Their Origin in Solar Cycles 23 and 24

Published:2024-08-21 Issue:8 Volume:15 Page:1016
ISSN:2073-4433
Container-title:Atmosphere
language:en
Short-container-title:Atmosphere

Author:

Miteva Rositsa¹^ORCID,Samwel Susan W.²^ORCID,Dechev Momchil¹^ORCID

Affiliation:

1. Institute of Astronomy and National Astronomical Observatory (IANAO), Bulgarian Academy of Sciences, 1784 Sofia, Bulgaria

2. National Research Institute of Astronomy and Geophysics (NRIAG), Helwan, Cairo 11421, Egypt

Abstract

The study presents the compilation of a comprehensive catalog of solar energetic protons (SEPs) in solar cycles (SCs) 23 and 24 (1996–2019) in 10 energy channels from about 20 to 100 MeV based on data from the Energetic and Relativistic Nuclei and Electron (ERNE) instrument aboard Solar and Heliospheric Observatory (SOHO). For comparison, we added previously reported SEP fluxes by a number of different sources. We identified the SEP-solar origin in terms of solar flares and coronal mass ejections and calculated the statistical correlations (Pearson and partial) as a function of the SEP energy.

Funder

SCOSTEP/PRESTO

Bulgarian Academy of Sciences

Publisher

MDPI AG

Link

https://www.mdpi.com/2073-4433/15/8/1016/pdf

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