Published 2008
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The Charge-to-Mass Dependence of Solar Energetic Particle Spectral Breaks
Abstract
Measurements of the energy spectra of SEP events over a broad energy range (~0.1 to 100 MeV/nuc) show that all large SEP events have spectral beaks organized by the charge-to-mass ratio (Q/M) of the ions. In this paper we present preliminary results of a multi-spacecraft study of the Q/M-dependence of spectral breaks in 11 SEP events and investigate whether the deduced Q/M dependence is correlated with other characteristics of the events.
Additional Information
Copyright Universidad Nacional Autónoma de México This work was supported by NASA under NNX06AC21G, NNG04GB55G, NNG04088G, and NAS5-12929. We appreciate the use of GOES data provided by NOAA.Attached Files
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Additional details
Identifiers
- Eprint ID
- 56895
- Resolver ID
- CaltechAUTHORS:20150422-163629154
Related works
- Describes
- http://adsabs.harvard.edu/abs/2008ICRC....1...99M (URL)
Funding
- NASA
- NNX06AC21G
- NASA
- NNG04GB55G
- NASA
- NAG5-12929
Dates
- Created
-
2015-04-29Created from EPrint's datestamp field
- Updated
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2020-03-09Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2008-15