Published 1969
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Cosmic-Ray Negatron and Positron Spectra Observed Near Fort Churchill in 1968
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Abstract
The differential energy spectra of cosmic-ray positrons and negatrons between 12 and 210 MeV have been measured with a balloon-borne magnetic spectrometer launched from Fort Churchill, Canada, in summer 1968. Since the geomagnetic cutoff varies with time, separate spectra for the local day and night intervals are presented. In addition, the corrections for atmospheric secondary electrons are discussed in detail. The solar modulation of the positron flux is compared with the modulation of cosmic-ray nuclei.
Additional Information
Work supported by the National Aeronautics and Space Administration under Grant Number NGL 05-002-007. Space Radiation Laboratory; SRL ID # 1969-07. Provided by the NASA Astrophysics Data System.Attached Files
Published - 1969-07.pdf
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1969-07.pdf
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Identifiers
- Eprint ID
- 44680
- Resolver ID
- CaltechAUTHORS:20140407-091516396
Related works
Funding
- NASA
- NGL 05-002-007
Dates
- Created
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2014-04-08Created from EPrint's datestamp field
- Updated
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2020-02-20Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Space Radiation Laboratory , Physics Department
- Series Name
- International Cosmic Ray Conference
- Series Volume or Issue Number
- 11
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1969-07