Published 2007
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Possible role of transients on the energy spectra of energetic particles at the solar wind termination shock
Abstract
We suggest that a series of merged interaction regions interacted with the solar wind termination shock for several years prior to its crossing by Voyager 1 in December 2004 and created the observed spectral shape of energetic particles. We also find that the charge-state of He with 3 to 70 MeV/nuc and O with 1 to 14 MeV/nuc is +1 and that the rigidity dependence of the diffusion coefficient from 170 MV to 2.7 GV is given by .
Additional Information
Copyright Universidad Nacional Autónoma de México We thank the Voyager MAG and Plasma teams for the use of their data. This work was supported by NASA under contract NAS7-03001.Attached Files
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Additional details
- Eprint ID
- 56694
- Resolver ID
- CaltechAUTHORS:20150415-152910440
- NASA
- NAS7-03001
- Created
-
2015-04-21Created from EPrint's datestamp field
- Updated
-
2020-02-20Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2008-10