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Comparing observations and expectations of SEP composition in the two December 2006 events

Cohen, C. M. S. and Mason, G. M. and Mewaldt, R. A. and Cummings, A. C. and Leske, R. A. and Stone, E. C. and Wiedenbeck, M. E. and von Rosenvinge, T. T. (2007) Comparing observations and expectations of SEP composition in the two December 2006 events. In: Proceedings of the 30th International Cosmic Ray Conference. Vol.1. Universidad Nacional Autónoma de México , Merida, Yucatan, Mexico, pp. 95-98. https://resolver.caltech.edu/CaltechAUTHORS:20150422-162304614

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Abstract

In early December 2006, a large active region (number 10930) rotated over the eastern limb of the Sun. As it crossed the disk, it produced 4 X-class flares and at least 3 halo coronal mass ejections. Two large SEP events were generated when the region was at ~E70 and ~W25 and were observed by several spacecraft, including ACE and STEREO. We have combined observations from the Solar Isotope Spectrometer (SIS) and the Ultra-Low Energy Isotope Spectrometer (ULEIS) on ACE and the Low Energy Telescope (LET) on STEREO for both SEP events. By integrating the SEP data over the duration of each event, the energy sp ectra for many heavy ion species (including Mg, Si, and Ca) can be analyzed in detail and the elemental SEP composition can be compared for the two events. We find significant differences in the composition of the two events, with the second event having a high Fe/O ratio, similar to that of impulsive SEP events. Both events are examined in terms of expectations from two prevailing models, but neither model completely predicts the observations.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/2008ICRC....1...95CADSArticle
ORCID:
AuthorORCID
Cohen, C. M. S.0000-0002-0978-8127
Mason, G. M.0000-0003-2169-9618
Mewaldt, R. A.0000-0003-2178-9111
Cummings, A. C.0000-0002-3840-7696
Leske, R. A.0000-0002-0156-2414
Stone, E. C.0000-0002-2010-5462
Wiedenbeck, M. E.0000-0002-2825-3128
Additional Information:Copyright Universidad Nacional Autónoma de México This work was supported by NASA and NSF under grants NAS5-12929, NAS5-03131, NNX-06AC21G, NNX06AC27G, and ATM-0454428.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAG5-12929
NASANAS5-03131
NASANNX06AC21G
NASANNX06AC27G
NSFATM-0454428
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2008-14
Record Number:CaltechAUTHORS:20150422-162304614
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150422-162304614
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:56893
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:24 Apr 2015 00:00
Last Modified:09 Mar 2020 13:19

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