Computer Science – Performance
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsm11a1581g&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SM11A-1581
Computer Science
Performance
0550 Model Verification And Validation, 2720 Energetic Particles: Trapped, 2740 Magnetospheric Configuration And Dynamics, 2744 Magnetotail, 2753 Numerical Modeling
Scientific paper
We present detailed comparisons of a time-dependent inner radiation belt model with in-situ proton observations made by a variety of spacecraft during solar cycle 23. The recently-developed model (Selesnick et al., 2007) computes proton intensities as a function of time and of the three adiabatic invariants in the inner belt, which we convert to the observable count rate in a detector at the location of the satellite by using instrument response functions. These comparisons and initial data-assimilation efforts suggest that the model performance can be improved especially during injections of solar protons, and at L-shells above 2.
Guild Timothy B.
Looper Mark
O'Brien Thomas P.
Selesnick Richard
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