Using the WSA Model to Test the Parker Spiral Approximation for SEP Event Magnetic Connections
Author:
Funder
AFOSR
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-016-0934-x.pdf
Reference58 articles.
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2. Arge, C.N., Luhmann, J.G., Odstrcil, D., Schrijver, C.J., Li, Y.: 2004, Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME. J. Atmos. Solar-Terr. Phys. 66, 1295. DOI .
3. AIP Conf. Proc.;C.N. Arge,2013
4. Bučík, R., Innes, D.E., Mall, U., Korth, A., Mason, G.M., Gómez-Herrero, R.: 2014, Multi-spacecraft observations of recurrent ${}^{3}\mathrm{He}$-rich solar energetic particles. Astrophys. J. 786, 71. DOI .
5. Chen, N., Bučík, R., Innes, D.E., Mason, G.M.: 2015, Case studies of multi-day ${}^{3}\mathrm{He}$-rich solar energetic particle periods. Astron. Astrophys. 580, A16. DOI .
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