Comparisons Between Numerically Determined and Observed Geomagnetic Cutoff Variations During Geomagnetic Storms

Details Comparisons Between Numerically Determined and Observed Geomagnetic Cutoff Variations During Geomagnetic Storms Comparisons Between Numerically Determined and Observed Geomagnetic Cutoff Variations During Geomagnetic Storms

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm23c..05k&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM23C-05

Statistics

Computation

2114 Energetic Particles (7514), 2740 Magnetospheric Configuration And Dynamics, 2753 Numerical Modeling, 2784 Solar Wind/Magnetosphere Interactions, 7984 Space Radiation Environment

Scientific paper

Geomagnetic cutoff variations during several storms are numerically
determined using trajectory computations in fields from (1) the
Tsyganenko 2005 geomagnetic field model and (2) the Lyon-Fedder-Mobarry
MHD magnetospheric simulation code. The modeled cutoffs are compared
with observed cutoffs obtained from SAMPEX energetic ion data.

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