Published September 15, 2000
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The morphology of anomalous cosmic rays in the outer heliosphere
Abstract
The well established cosmic ray transport equation describes the physics of cosmic ray modulation in the heliosphere and is thought to be complete. Its solution for anomalous cosmic rays has special characteristics due to the local acceleration of these particles at the solar wind termination shock. Some of these characteristics are demonstrated here, namely effects by the strength of the shock, shock drift, the cutoff in the spectrum at the shock, species scaling, drift, and ionization.
Additional Information
© 2000 American Institute of Physics. Issue Date: 15 September 2000. This work was supported by NASA at Caltech (contract NAS7-918).Attached Files
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Additional details
- Eprint ID
- 28378
- Resolver ID
- CaltechAUTHORS:20111208-164736889
- NAS7-918
- NASA
- Created
-
2011-12-09Created 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
- 528
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2000-26