Stone, E. C. and Cummings, A. C. and Webber, W. R.
(1995)
Evolution of the Energy Spectra of Anomalous Cosmic Rays in the Outer Heliosphere and the Distance to the Solar Wind Termination Shock.
In:
Proceedings of the 24th International Cosmic Ray Conference.
Vol.4.
International Union of Pure and Applied Physics
, pp. 792-795.
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Abstract
Using data from the Voyager 1 and 2 (Vl and V2) spacecraft, we examine
the energy spectra of anomalous cosmic rays (ACRs) for three time periods
in 1993 - 1994. We use a spherically-symmetric model of the propagation
of ACRs in the heliosphere to derive the energy spectrum of ACRs at the
solar wind termination shock and the shock's location. We find that in late
1994 the shock strength has a value of 2.40 ± 0.12 and is located at 84.2
(-2.2, +2.6) AU.
Item Type: | Book Section |
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Additional Information: | © IUPAP. Provided by the NASA Astrophysics Data System.
This work
was supported in part by NASA under
contract NAS7-9I8 and grant NAGWI9I9. |
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Group: | Space Radiation Laboratory |
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Funders: | Funding Agency | Grant Number |
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NASA | NAS7-9I8 | NASA | NAGWI9I9 |
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Other Numbering System: | Other Numbering System Name | Other Numbering System ID |
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Space Radiation Laboratory | 1995-20 |
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Record Number: | CaltechAUTHORS:20140616-163928405 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140616-163928405 |
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Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 46291 |
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Collection: | CaltechAUTHORS |
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Deposited By: |
Deborah Miles
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Deposited On: | 24 Jun 2014 18:11 |
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Last Modified: | 20 Feb 2020 14:33 |
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