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A model of solar energtic particles for use in calculating LET spectra developed from ONR-604 dataA model of Solar Energetic Particles (SEP) has been developed and is applied to solar flares during the 1990/1991 Combined Release and Radiation Effects Satellite (CRRES) mission using data measured by the University of Chicago instrument, ONR-604. The model includes the time-dependent behavior, heavy-ion content, energy spectrum and influence, and can accurately represent the observed SEP events in the energy range between 40 to 500 MeV/nucleon. Results are presented for the March and June, 1991 flare periods.
Document ID
19940039097
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Chen, J.
(Louisiana State Univ. Baton Rouge, LA, US, United States)
Chenette, D.
(Lockheed Palo Alto Research Laboratory, Palo Alto, CA US, United States)
Guzik, T. G.
(Louisiana State Univ. Baton Rouge, LA, US, United States)
Garcia-Munoz, M.
(Univ. of Chicago, Chicago, IL US, United States)
Pyle, K. R.
(Univ. of Chicago, Chicago, IL US, United States)
Sang, Y.
(Louisiana State Univ. Baton Rouge, LA, US, United States)
Wefel, J. P.
(Louisiana State Univ. Baton Rouge, LA, US, United States)
Date Acquired
August 16, 2013
Publication Date
October 1, 1994
Publication Information
Publication: Life Sciences and Space Research 25 (2) Radiation Biology: Topical Meeting of the COSPAR Interdisciplinary Scientific Commission F of the COSPAR 29th Plenary Meeting, Washington, DC, Aug. 28-Sep. 5, 1
Volume: 14
Issue: 10
ISSN: 0273-1177
Subject Category
Space Radiation
Accession Number
94A62546
Funding Number(s)
CONTRACT_GRANT: F19628-90-K-0026
CONTRACT_GRANT: NAG5-706
CONTRACT_GRANT: F196 28-90-C-0101
CONTRACT_GRANT: NAGW-2368
CONTRACT_GRANT: N00014-90-J-1466
CONTRACT_GRANT: F19628-90-K-0025
Distribution Limits
Public
Copyright
Other

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