A 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.


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    Title :

    A model of solar energtic particles for use in calculating LET spectra developed from ONR-604 data


    Contributors:
    Chen, J. (author) / Chenette, D. (author) / Guzik, T. G. (author) / Garcia-Munoz, M. (author) / Pyle, K. R. (author) / Sang, Y. (author) / Wefel, J. P. (author)


    Publication date :

    1994-10-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English






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