Marshall, F. E. and Stone, E. C. (1976) Persistent Sunward Flow of ~1.6 MeV Protons at 1 Au. Transactions - American Geophysical Union, 57 (12). p. 980. ISSN 0002-8606. doi:10.1029/EO057i012p00893. https://resolver.caltech.edu/CaltechAUTHORS:20140205-082430682
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Abstract
The anisotropy of 1.3 to 2.3 MeV protons has been measured with the Caltech Electron/Isotope Spectrometer aboard IMP-7 for periods between prompt solar particle events from 72/273 to 74/2. The diffusive anisotropy, which has been computed by subtracting the independently determined. convective anisotropy from the observed anisotropy, is predominantly directed toward the sun with a typical radial component of 14%.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1976 American Geophysical Union. | |||||||||
| Group: | Space Radiation Laboratory | |||||||||
| Issue or Number: | 12 | |||||||||
| DOI: | 10.1029/EO057i012p00893 | |||||||||
| Record Number: | CaltechAUTHORS:20140205-082430682 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140205-082430682 | |||||||||
| Official Citation: | Anonymous (1976), Abstracts [Fall Meeting, 1976], Eos Trans. AGU, 57(12), 893–1033, doi:10.1029/EO057i012p00893 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 43664 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 25 Feb 2014 21:07 | |||||||||
| Last Modified: | 10 Nov 2021 16:41 |
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