Physics
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jgr....87.5943o&link_type=abstract
Journal of Geophysical Research, vol. 87, Aug. 1, 1982, p. 5943-5948. Research supported by the McDonnell Douglas Independent R
Physics
23
Atmospheric Electricity, Geomagnetism, Magnetic Field Configurations, Magnetic Variations, Magnetospheric Instability, Sudden Storm Commencements, Dynamic Models, Electric Field Strength, Geomagnetic Tail, Interplanetary Magnetic Fields, Magnetopause, Ring Currents, Solar Terrestrial Interactions, Solar Wind
Scientific paper
A quantitative vector representation of the magnetospheric field was developed specifically for the complex event of July 29, 1977. The magnetic field associated with each of the three major magnetospheric current systems was 'controlled' by solar wind and interplanetary field parameters and a magnetic index. This dynamic field model was compared with observed field data and found to be in good agreement. The procedures developed for quantitatively modeling time varying magnetospheric phenomena are general, and eventually it should be possible to use them to 'predict' some aspects of magnetospheric behavior.
Olson W. P.
Pfitzer K. A.
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