Published 2013
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Solar energetic particles and their variability from the sun and beyond
Chicago
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Abstract
With the onset of solar cycle 24 activity STEREO and near-Earth spacecraft are now measuring many multi-spacecraft solar particle events. We present examples of time-intensity distributions, energy spectra, fits to longitude distributions, a combined imaging/in-situ study, and MHD modeling of one event. Implications of these new results are discussed.
Additional Information
© 2013 AIP Publishing LLC. This work was supported by NASA at Caltech under grants NNX8AI11G and NNX06AC21G, and under subcontract SA2715-26309 from UC Berkeley under NASA contract NAS5-03131; at JHU/APL by NASA grant NNX10AT75G, UC Berkeley subcontract SA4889-26309, and NSF SHINE grant 1156138; and at NRL under grant NNH11AR711. We appreciate the availability of GOES data from NOAA, EPHIN data from the University of Kiel, and LASCO data from the Catholic University website.Attached Files
Published - APC000116.pdf
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Additional details
- Eprint ID
- 39109
- Resolver ID
- CaltechAUTHORS:20130626-134934610
- NASA
- NNX8AI11G
- NASA
- NNX06AC21G
- NASA
- SA2715-26309
- NASA
- NAS5-03131
- NASA
- NNX10AT75G
- NASA
- SA4889-26309
- NSF
- AGS-1156138
- NASA
- NNH11AR711
- Created
-
2013-07-23Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Series Name
- AIP Conference Proceedings
- Series Volume or Issue Number
- 1539
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2013-21