Source Energy Spectrum of the 17 May 2012 GLE

Author:

Pérez-Peraza Jorge1,Márquez-Adame Juan C.1,Miroshnichenko Leonty23,Velasco-Herrera Victor1ORCID

Affiliation:

1. Instituto de Geofísica; Universidad Nacional Autónoma de México; México City Mexico

2. Pushkov Institute of Terrestrial Magnetism; Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences; Moscow Russia

3. Skobeltsyn Institute of Nuclear Physics; Lomonosov Moscow State University; Moscow Russia

Funder

Consejo Nacional de Ciencia y Tecnología

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference64 articles.

1. Fermi-LAT observations of high-energy behind-the-limb solar flares;Ackermann;The Astrophysical Journal,2017

2. Spectrum of solar cosmic rays in the source taking into account their coronal propagation;Álvarez-Madrigal;Soviet Astronomy,1986

3. Analysis of ground level enhancements (GLE): Extreme solar energetic particle events have hard spectra;Asvestari;Advances in Space Research,2017

4. Augusto , C. R. A. Kopenkin , V. Navia , C. E. Felicio , A. C. S. Freire , F. Pinto , A. C. S. 2013 Was the GLE on May 17, 2012 linked with the M5.1-class flare the first in the 24th solar cycle? arXiv:1301 7055 Astroph SR

5. Balabin , Yu. V. Germanenko , A. V. Vashenyuk , E. V. Gvozdevsky , B. B. 2013 The first GLE of the new 24th solar cycle

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