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Persistent Sunward Flow of ~1.6 MeV Protons at 1 Au

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. 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
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/EO057i012p00893DOIAbstracts
http://onlinelibrary.wiley.com/doi/10.1029/EO057i012p00893/abstractPublisherAbstracts
ORCID:
AuthorORCID
Stone, E. C.0000-0002-2010-5462
Additional Information:© 1976 American Geophysical Union.
Group:Space Radiation Laboratory
Issue or Number:12
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:20 Feb 2020 14:33

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