Flux of Cosmic Ray Electrons Between 17 and 63 MeV
The flux of cosmic-ray electrons in the energy interval of 17-63 MeV was measured in three high-altitude balloon flights during the summer 1967 near Fort Churchill, Manitoba. The average flux was found to be 0.3±0.2 electrons/m^2 sec sr MeV. Implications of this result on models of the origin of ga...
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ftcaltechauth:oai:authors.library.caltech.edu:xebfn-sjn93 2024-06-23T07:52:07+00:00 Flux of Cosmic Ray Electrons Between 17 and 63 MeV Israel, Martin H. Vogt, Rochus E. 1968-05-06 https://doi.org/10.1103/PhysRevLett.20.1053 unknown American Physical Society https://doi.org/10.1103/PhysRevLett.20.1053 oai:authors.library.caltech.edu:xebfn-sjn93 eprintid:44632 resolverid:CaltechAUTHORS:20140403-101033514 info:eu-repo/semantics/openAccess Other Physical Review Letters, 20(19), 1053-1056, (1968-05-06) info:eu-repo/semantics/article 1968 ftcaltechauth https://doi.org/10.1103/PhysRevLett.20.1053 2024-06-12T06:19:42Z The flux of cosmic-ray electrons in the energy interval of 17-63 MeV was measured in three high-altitude balloon flights during the summer 1967 near Fort Churchill, Manitoba. The average flux was found to be 0.3±0.2 electrons/m^2 sec sr MeV. Implications of this result on models of the origin of galactic cosmic-ray electrons and their solar modulation are discussed. © 1968 American Physical Society. Received 28 March 1968. We wish to thank Dr. K. Beuermann, Professor L. Davis, Professor E. Stone, and Mr. C. Rice for stimulating discussions. Also, we gratefully acknowledge the efforts of Mr. C. Rice, Mr. W. Blodgett, and Mr. M. Casteel, who assisted in various phases of construction, operation, and data reduction. We also express our appreciation to the staff of the Caltech synchrotron for use of their facilities for the calibration of our detector. * Work supported by the National Aeronautics and Space Administration under Grant No. NsG-426. Published - PhysRevLett.20.1053.pdf Article in Journal/Newspaper Churchill Caltech Authors (California Institute of Technology) Fort Churchill ENVELOPE(-94.079,-94.079,58.756,58.756) Physical Review Letters 20 19 1053 1056 |
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Caltech Authors (California Institute of Technology) |
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The flux of cosmic-ray electrons in the energy interval of 17-63 MeV was measured in three high-altitude balloon flights during the summer 1967 near Fort Churchill, Manitoba. The average flux was found to be 0.3±0.2 electrons/m^2 sec sr MeV. Implications of this result on models of the origin of galactic cosmic-ray electrons and their solar modulation are discussed. © 1968 American Physical Society. Received 28 March 1968. We wish to thank Dr. K. Beuermann, Professor L. Davis, Professor E. Stone, and Mr. C. Rice for stimulating discussions. Also, we gratefully acknowledge the efforts of Mr. C. Rice, Mr. W. Blodgett, and Mr. M. Casteel, who assisted in various phases of construction, operation, and data reduction. We also express our appreciation to the staff of the Caltech synchrotron for use of their facilities for the calibration of our detector. * Work supported by the National Aeronautics and Space Administration under Grant No. NsG-426. Published - PhysRevLett.20.1053.pdf |
format |
Article in Journal/Newspaper |
author |
Israel, Martin H. Vogt, Rochus E. |
spellingShingle |
Israel, Martin H. Vogt, Rochus E. Flux of Cosmic Ray Electrons Between 17 and 63 MeV |
author_facet |
Israel, Martin H. Vogt, Rochus E. |
author_sort |
Israel, Martin H. |
title |
Flux of Cosmic Ray Electrons Between 17 and 63 MeV |
title_short |
Flux of Cosmic Ray Electrons Between 17 and 63 MeV |
title_full |
Flux of Cosmic Ray Electrons Between 17 and 63 MeV |
title_fullStr |
Flux of Cosmic Ray Electrons Between 17 and 63 MeV |
title_full_unstemmed |
Flux of Cosmic Ray Electrons Between 17 and 63 MeV |
title_sort |
flux of cosmic ray electrons between 17 and 63 mev |
publisher |
American Physical Society |
publishDate |
1968 |
url |
https://doi.org/10.1103/PhysRevLett.20.1053 |
long_lat |
ENVELOPE(-94.079,-94.079,58.756,58.756) |
geographic |
Fort Churchill |
geographic_facet |
Fort Churchill |
genre |
Churchill |
genre_facet |
Churchill |
op_source |
Physical Review Letters, 20(19), 1053-1056, (1968-05-06) |
op_relation |
https://doi.org/10.1103/PhysRevLett.20.1053 oai:authors.library.caltech.edu:xebfn-sjn93 eprintid:44632 resolverid:CaltechAUTHORS:20140403-101033514 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1103/PhysRevLett.20.1053 |
container_title |
Physical Review Letters |
container_volume |
20 |
container_issue |
19 |
container_start_page |
1053 |
op_container_end_page |
1056 |
_version_ |
1802643335118061568 |