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Correlation of Upper-Atmospheric 7-Be with Solar Energetic Particle EventsA surprisingly large concentration of radioactive 7-Be was observed in the upper atmosphere at altitudes above 320 km on the LDEF satellite that was recovered in January 1990. We report on follow-up experiments on Russian spacecraft at altitudes of 167 to 370 km during the period of 1996 to 1999, specifically designed to measure 7-Be concentrations in low earth orbit. Our data show a significant correlation between the 7-Be concentration and the solar energetic proton fluence at Earth, but not with the overall solar activity. During periods of low solar proton fluence, the concentration is correlated with the galactic cosmic ray fluence. This indicates that spallation of atmospheric N by both solar energetic particles and cosmic rays is the primary source of 7-Be in the ionosphere.
Document ID
20010037913
Acquisition Source
Marshall Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Phillips, G. W.
(Naval Research Lab. Washington, DC United States)
Share, G. H.
(Naval Research Lab. Washington, DC United States)
King, S. E.
(Naval Research Lab. Washington, DC United States)
August, R. A.
(Naval Research Lab. Washington, DC United States)
Tylka, A. J.
(Naval Research Lab. Washington, DC United States)
Adams, J. H., Jr.
(Naval Research Lab. Washington, DC United States)
Panasyuk, M. I.
(Moscow State Univ. Russia)
Nymmik, R. A.
(Moscow State Univ. Russia)
Kuzhevskij, B. M.
(Moscow State Univ. Russia)
Kulikauskas, V. S.
(Moscow State Univ. Russia)
Rose, M. Franklin
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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