Beuermann, K. P. and Rice, C. J. and Stone, E. C. and Vogt, R. E.
(1969)
Cosmic-Ray Negatron and Positron Spectra Between 12 and 220 MeV.
Physical Review Letters, 22
(9).
pp. 412-415.
ISSN 0031-9007.
doi:10.1103/PhysRevLett.22.412.
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Abstract
The interplanetary negatron and positron spectra from 12 to 220 MeV have been determined with a balloon-borne magnetic spectrometer. The observed charge ratio e^+(e^+ + e^−)≈0.3 indicates that the flux most likely consists of a mixture of "primary" negatrons and interstellar "secondary" negatrons and positrons. We deduce an absolute solar modulation of the interstellar positron flux which decreases with decreasing magnetic rigidity below about 80 MV.
Item Type: | Article |
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Additional Information: | © 1969 American Physical Society.
Received 23 December 1968.
Work supported by the National Aeronautics and
Space Administration under Grant No. NGL-05-002-007.
Space Radiation Laboratory.
SRL ID #: 1969-04. |
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Group: | Space Radiation Laboratory |
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Funders: | Funding Agency | Grant Number |
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NASA | NGL-05-002-007 |
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Other Numbering System: | Other Numbering System Name | Other Numbering System ID |
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Space Radiation Laboratory | 1969-04 |
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Issue or Number: | 9 |
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DOI: | 10.1103/PhysRevLett.22.412 |
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Record Number: | CaltechAUTHORS:20140407-083050683 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140407-083050683 |
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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: | 44674 |
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Collection: | CaltechAUTHORS |
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Deposited By: |
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Deposited On: | 07 Apr 2014 16:29 |
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Last Modified: | 10 Nov 2021 16:55 |
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