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The Source Material for Large Solar Energetic Particle Events

Mewaldt, R. A. and Cohen, C. M. S. and Mason, G. M. (2006) The Source Material for Large Solar Energetic Particle Events. In: Solar Eruptions and Energetic Particles. Geophysical Monograph Series. No.165. American Geophysical Union , Washington, DC, pp. 115-125. ISBN 9780875904306. https://resolver.caltech.edu/CaltechAUTHORS:20150324-092218323

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Abstract

We review evidence regarding the origin of material accelerated in large, gradual solar energetic particle (SEP) events. According to the two-class paradigm in place at the start of solar cycle 23, impulsive SEP events accelerate heated flare material, while gradual SEP events are accelerated out of the solar wind by shocks driven by fast coronal mass ejections (CMEs). However, new data from solar cycle 23 has shown that the energetic ions in gradual events often include composition signatures associated with impulsive events, including enrichments in ^3He, heavy elements such as Fe, and ionic charge states indicative of~ 10 MK temperatures. In addition, gradual SEP events differ in composition from bulk solar wind in several key respects, implying that solar wind is not the principal seed population for these events. Several lines of evidence show that CME-driven shocks accelerate principally suprathennal ions with velocities several times that of the solar wind. The suprathermal pool incorporates ions from impulsive solar flares and previous gradual events, CIR events, pickup ions, CME ejecta, and the suprathermal tail of the solar wind. This paper reviews evidence for the sources of ions accelerated in gradual SEP events, considers the composition and available densities of suprathermal ions, and describes models that attempt to account for the surprisingly variable composition of gradual SEP events. We find that below ~1 MeV/nucleon almost all events are Fe-rich compared to the average 5 to 12 MeV/nucleon SEP composition. Iron-rich SEP events above 10 Me V/nucleon occur mainly during periods when the intensity of suprathermal iron in the inner heliosphere is high, due mainly to previous gradual events.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/165GM12DOIArticle
http://onlinelibrary.wiley.com/doi/10.1029/165GM12/summaryPublisherArticle
ORCID:
AuthorORCID
Mewaldt, R. A.0000-0003-2178-9111
Cohen, C. M. S.0000-0002-0978-8127
Mason, G. M.0000-0003-2169-9618
Additional Information:© 2006 American Geophysical Union. This work was supported by NASA under grants NNG04GB55G, NNG04088G, and NAG5-12929. We appreciate discussions with Berndt Klecker, Eberhard Moebius, and Edward Stone, and figures provided by Berndt Klecker, Allan Labrador, Mark Popecki, and Mark Wiedenbeck. We thank the local organizing committee for a very informative and enjoyable conference.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANNG04GB55G
NASANNG04088G
NASANAG5-12929
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2006-03
Series Name:Geophysical Monograph Series
Issue or Number:165
Record Number:CaltechAUTHORS:20150324-092218323
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150324-092218323
Official Citation:Mewaldt, R. A., Cohen, C. M. S. and Mason, G. M. (2006) The Source Material for Large Solar Energetic Particle Events, in Solar Eruptions and Energetic Particles (eds N. Gopalswamy, R. Mewaldt and J. Torsti), American Geophysical Union, Washington, D. C.. doi: 10.1029/165GM12
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:56009
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:24 Mar 2015 17:43
Last Modified:22 Nov 2019 09:58

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