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On the Differences in Composition between Solar Energetic Particles and Solar Wind

Mewaldt, R. A. and Cohen, C. M. S. and Mason, G. M. and Cummings, A. C. and Desai, M. I. and Leske, R. A. and Raines, J. and Stone, E. C. and Wiedenbeck, M. E. and von Rosenvinge, T. T. and Zurbuchen, T. H. (2007) On the Differences in Composition between Solar Energetic Particles and Solar Wind. Space Science Reviews, 130 (1-4). pp. 207-219. ISSN 0038-6308. http://resolver.caltech.edu/CaltechAUTHORS:20100506-100356849

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Abstract

Although the average composition of solar energetic particles (SEPs) and the bulk solar wind are similar in a number of ways, there are key differences which imply that solar wind is not the principal seed population for SEPs accelerated by coronal mass ejection (CME) driven shocks. This paper reviews these composition differences and considers the composition of other possible seed populations, including coronal material, impulsive flare material, and interplanetary CME material.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/s11214-007-9187-1DOIArticle
http://www.springerlink.com/content/p054752525607622/PublisherArticle
ORCID:
AuthorORCID
Cohen, C. M. S.0000-0002-0978-8127
Mason, G. M.0000-0003-2169-9618
Additional Information:© 2007 Springer Science+Business Media, Inc. Received: 5 February 2007; accepted: 4 April 2007; published online: 26 May 2007. We are grateful to the local organizing committee at ISSI for their contributions to a very successful and enjoyable Symposium. This work was supported by NASA under grants NNG04GB55G, NNG04088G, and NAG5-12929.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANNG04GB55G
NASANNG04088G
NASANAG5-12929
Subject Keywords:Sun: particle emission - Sun: solar wind - Sun: coronal mass ejections (CMEs); Sun: abundances; Sun: flares; Acceleration of particles
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2007-08
Record Number:CaltechAUTHORS:20100506-100356849
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20100506-100356849
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:18163
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:06 May 2010 19:01
Last Modified:12 Sep 2017 03:42

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