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Electron contamination in a mid-latitude soft X-ray astronomy experiment during an intense magnetic stormA large area X-ray sky survey payload was launched from White Sands Missile Range (106 deg W 32 deg N) on 1 Nov. 1972 at 0530 hours U.T. The launch time coincided with intense geomagnetic activity (3 hour K sub p index = 8) following a solar flare. The data have been analyzed to determine possible contamination of X-ray data by large fluxes of low energy electrons that can precipitate down to low altitudes during magnetic storms. There is clear evidence in the data for low energy electrons of 10 - 50 keV contributing appreciably at about 200 km altitude in the 1 - 10 keV X-ray energy channels of the proportional counters used for the X-ray observations. The McIlwain parameters L and B for this altitude at White Sands are 1.25 and 0.46G, respectively.
Document ID
19740020140
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Naranan, S.
(Naval Research Lab. Washington, DC, United States)
Friedman, H.
(Naval Research Lab. Washington, DC, United States)
Fritz, G.
(Naval Research Lab. Washington, DC, United States)
Henry, R. C.
(Naval Research Lab. Washington, DC, United States)
Shulman, S.
(Naval Research Lab. Washington, DC, United States)
Date Acquired
August 7, 2013
Publication Date
May 1, 1974
Publication Information
Publication: NASA. Goddard Space Flight Center Proc. of the Workshop on Electron Contamination in X-ray Astronomy Expt.
Subject Category
Space Radiation
Accession Number
74N28253
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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