Characteristics of SEP Events and Their Solar Origin During the Evolution of Active Region NOAA 10069-Reference-Cited by-同舟云学术

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Characteristics of SEP Events and Their Solar Origin During the Evolution of Active Region NOAA 10069

Published:2019-01 Issue:1 Volume:294 Page:
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Kashapova L. K.^ORCID,Miteva R.^ORCID,Myagkova I. N.^ORCID,Bogomolov A. V.

Funder

the Russian Foundation for Basic Research

The National Science Fund of Bulgaria

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/article/10.1007/s11207-019-1400-3/fulltext.html

Reference37 articles.

1. Aschwanden, M.J., Caspi, A., Cohen, C.M.S., Holman, G., Jing, J., Kretzschmar, M., Kontar, E.P., McTiernan, J.M., Mewaldt, R.A., O’Flannagain, A., Richardson, I.G., Ryan, D., Warren, H.P., Xu, Y.: 2017, Global energetics of solar flares. V. Energy closure in flares and coronal mass ejections. Astrophys. J. 836, 17. DOI . ADS .

2. Bastian, T.S., Benz, A.O., Gary, D.E.: 1998, Radio emission from solar flares. Annu. Rev. Astron. Astrophys. 36, 131. DOI . ADS .

3. Bogomolov, A.V., Kashapova, L.K., Myagkova, I.N., Tsap, Y.T.: 2014, Dynamics of the hard X-ray, gamma-ray, and microwave emission of solar flares produced by the active region NOAA 0069 in August 2002. Astron. Rep. 58, 156. DOI . ADS .

4. Bronarska, K., Michalek, G.: 2017, Characteristics of active regions associated to large solar energetic proton events. Adv. Space Res. 59, 384. DOI . ADS .

5. Cane, H.V., Erickson, W.C., Prestage, N.P.: 2002, Solar flares, type III radio bursts, coronal mass ejections, and energetic particles. J. Geophys. Res. 107, 1315. DOI . ADS .

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1. Characteristics of SEPs during solar cycles 21–24;Journal of Astrophysics and Astronomy;2020-03-11

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