Published 1995
| Version Published
Book Section - Chapter
Open
Interpretation of the Low-Energy Cosmic Ray Antiproton/Proton Ratio
Creators
Contributors
Others:
Abstract
We examine the solar modulation of cosmic ray protons and antiprotons, and discuss the resulting effects on the low-energy antiproton/proton ratio at 1 AU. We find that the anitiproton/proton ratio at energies >3 GeV is a useful diagnostic of cosmic ray transport in the Galaxy. However, at energies
Additional Information
© IUPAP. Provided by the NASA Astrophysics Data System. This work was funded by NASA under NAGW-1919. One of us (AL) is grateful for a NASA Graduate Fellowship. We thank W.R. Webber, T. Gaisser, R. Shaeffer, and R. Streitmatter for useful discussions.Attached Files
Published - 1995-26.pdf
Files
1995-26.pdf
Files
(887.5 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:7aa784ff8f08d0effcc484c665870027
|
887.5 kB | Preview Download |
Additional details
Identifiers
- Eprint ID
- 46317
- Resolver ID
- CaltechAUTHORS:20140617-163638959
Related works
- Describes
- http://adsabs.harvard.edu/abs/1995ICRC....3...68L (URL)
Funding
- NASA
- NAGW-1919
- NASA Graduate Fellowship
Dates
- Created
-
2014-07-07Created from EPrint's datestamp field
- Updated
-
2020-02-20Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1995-26