Cummings, A. C. and Stone, E. C. (2007) Possible role of transients on the energy spectra of energetic particles at the solar wind termination shock. In: Proceedings of the 30th International Cosmic Ray Conference. Vol.1. Universidad Nacional Autónoma de México , Merida, Yucatan, Mexico, pp. 827-830. https://resolver.caltech.edu/CaltechAUTHORS:20150415-152910440
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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 .
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| 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. | ||||||
| Group: | Space Radiation Laboratory | ||||||
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| Record Number: | CaltechAUTHORS:20150415-152910440 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20150415-152910440 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 56694 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Deborah Miles | ||||||
| Deposited On: | 21 Apr 2015 20:56 | ||||||
| Last Modified: | 20 Feb 2020 14:33 |
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