Published August 28, 2007
| Published
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Radiation risks from large solar energetic particle events
Abstract
Solar energetic particles (SEPs) constitute a radiation hazard to both humans and hardware in space. Over the past few years there have been significant advances in our knowledge of the composition and energy spectra of SEP events, leading to new insights into the conditions that contribute to the largest events. This paper summarizes the energy spectra and frequency of large SEP events, and discusses the interplanetary conditions that affect the intensity of the largest events.
Additional Information
© 2007 American Institute of Physics This work was supported by NASA under NAS5-03131, NAG5-12929, NNG04GB55G and NNX06AC21G. We appreciate the use of GOES data provided by NOAA and thank the organizers for an excellent conference.Attached Files
Published - MEWaipcp07.pdf
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MEWaipcp07.pdf
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Additional details
- Eprint ID
- 8657
- Resolver ID
- CaltechAUTHORS:MEWaipcp07
- NASA
- NAS5-03131
- NASA
- NAG5-12929
- NASA
- NNG04GB55G
- NASA
- NNX06AC21G
- Created
-
2007-09-03Created from EPrint's datestamp field
- Updated
-
2023-06-01Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Series Name
- AIP Conference Proceedings
- Series Volume or Issue Number
- 932
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2007-06