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Impulsive Flare Material: A Seed Population for Large Solar Particle Events?

Mewaldt, R. A. and Cohen, C. M. S. and Mason, G. M. and Desai, S. and Leske, R. A. and Mazur, J. E. and Stone, E. C. and von Rosenvinge, T. T. and Wiedenbeck, M. E. (2003) Impulsive Flare Material: A Seed Population for Large Solar Particle Events? In: Proceedings of the 28th International Cosmic Ray Conference. Vol.6. International Union of Applied Physics , Tokyo, Japan, pp. 3229-3232. http://resolver.caltech.edu/CaltechAUTHORS:20150403-094053625

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Abstract

It has been suggested that gradual solar energetic particle (SEP) events enriched in ^3He and Fe result from the shock acceleration of remnant interplanetary material from previous impulsive flares. We test this hypothesis by comparing the number densities of Fe ions during quiet periods, ^3He-rich periods, and Ferich SEP events. We find that there is not a sufficient density of suprathermal Fe during typical quiet periods (or ^3He-rich periods) to account for the overall enrichment of Fe in and suggest other possibilities for interpreting these events.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/full/2003ICRC....6.3229MADSArticle
ORCID:
AuthorORCID
Cohen, C. M. S.0000-0002-0978-8127
Mason, G. M.0000-0003-2169-9618
Additional Information:Copyright Universal Academy Press Inc. Supported by NASA at participating institutions.
Group:Space Radiation Laboratory
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2003-12
Record Number:CaltechAUTHORS:20150403-094053625
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150403-094053625
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:56338
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:03 Apr 2015 19:20
Last Modified:14 Sep 2017 22:48

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