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Splash Albedo Protons Between 4 and 315 MeV at High and Low Geomagnetic Latitudes

Wenzel, K.-P. and Stone, E. C. and Vogt, R. E. (1975) Splash Albedo Protons Between 4 and 315 MeV at High and Low Geomagnetic Latitudes. Journal of Geophysical Research A, 80 (25). pp. 3580-3584. ISSN 0148-0227. http://resolver.caltech.edu/CaltechAUTHORS:20140410-142447456

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Abstract

The differential energy spectrum of splash albedo protons has been measured at high geomagnetic latitude near Fort Churchill, Manitoba, at three periods of the solar cycle in 1966, 1967, and 1969 and at low latitude near Palestine, Texas, in 1967 by using a balloon-borne solid state detector telescope. We observed splash albedo proton fluxes between 4 and 315 MeV of 81 ± 11, 70 ± 11, and 48 ± 8 protons/(m² s sr) at high latitude in 1966, 1967, and 1969 and of 37 ± 9 protons/(m² s sr) at low latitude in 1967. The decreases from 1966 to 1969 are due to solar modulation of the cosmic ray parent nuclei. The albedo spectrum shows a similar shape for both latitudes. The difference in intensity can be explained by different local geomagnetic cutoffs; i.e., a significant contribution to the splash albedo flux arises from primary particles with rigidity below 4.5 GV. The splash albedo flux near Fort Churchill is consistent with corresponding fluxes previously reported near 53°-55°N. The flux below 100 MeV near Palestine is significantly lower than that reported by Verma (1967).


Item Type:Article
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http://dx.doi.org/10.1029/JA080i025p03580 DOIArticle
http://onlinelibrary.wiley.com/doi/10.1029/JA080i025p03580/abstractPublisherArticle
Contact Email Address:dmiles@caltech.edu
Additional Information:© 1975 by the American Geophysical Union. Received October 1, 1974; revised February 14, 1975; accepted March 6, 1975. We thank T. L. Garrard for his assistance, especially during the data analysis. We are very grateful to W. E. Althouse for the design of the electronics and his support during measurements. J. A. Lockwood kindly supplied the Mount Washington neutron monitor data. Most of this work was performed during a stay of one of the authors (K.P. W.) at the California Institute of Technology, supported by a NASA International Fellowship. It was completed as part of a Ph.D. thesis at the University of Heidelberg in Germany. This research was supported in part by the National Aeronautics and Space Administration under grant NGR-05-002-160. The Editor thanks W. R. Webber and R. S. White for their assistance in evaluating this paper. Space Radiation Laboratory SRL ID #: 1975-15.
Group:Space Radiation Laboratory
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Funding AgencyGrant Number
NASANGR-05-002-160
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Space Radiation Laboratory1975-15
Record Number:CaltechAUTHORS:20140410-142447456
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140410-142447456
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ID Code:44872
Collection:CaltechAUTHORS
Deposited By: SWORD User
Deposited On:11 Apr 2014 17:52
Last Modified:11 Apr 2014 17:52

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