Characteristics of ground-level enhancement-associated solar flares, coronal mass ejections, and solar energetic particles

Author:

Firoz K. A.1,Cho K.-S.1,Hwang J.1,Phani Kumar D. V.1,Lee J. J.1,Oh S. Y.2,Kaushik Subhash C.3,Kudela Karel4,Rybanský Milan4,Dorman Lev I.5

Affiliation:

1. Solar and Space Weather Research Group; Korea Astronomy and Space Science Institute; Daejeon South Korea

2. Bartol Research Institute; University of Delaware; Newark Delaware USA

3. School of Studies in Physics; Jiwaji University; Gwalior India

4. Institute of Experimental Physics; Slovak Academy of Sciences; Košice Slovakia

5. Israel Cosmic Ray and Space Weather Center and Emilio Segre' Observatory, Technion and Israel Space Agency; Qazrin Israel

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference50 articles.

1. A search for CMEs associated with big flares;Andrews;Sol. Phys.,2003

2. Properties of solar X-ray flares and proton event forecasting;Belov;Adv. Space Res.,2009

3. Solar cosmic rays during the extremely high ground level enhancement on 23 February1956;Belov;Ann. Geophys.,2005

4. Relativistic solar neutrons and protons on 28 October 2003;Bieber;Geophys. Res. Lett.,2005

5. Braun , I. 2005 Solar modulation of cosmic rays in the range from 10 to 20 GeV Conf. Pap. Int. Cosmic Ray Conf. XXIX 2 135 138

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