Physics
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37..379s&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 37, April 1989, p. 379-384.
Physics
17
Earth Magnetosphere, Image Processing, Magnetic Storms, Solar Radiation, Pixels, Spatial Resolution, Time Dependence
Scientific paper
The possibility of imaging the earth's magnetosphere in resonantly scattered sunlight is discussed. Resonant scattering solar emissions near 834 A by O(+) are found to be a possible means of viewing magnetospheric plasma and tracing processes within the magnetosphere. Simulations of 834-A images observed from a lunar orbit are used to study the radiation belts and plasma sheet. It is suggested that, using near-term technology, useful images could be made in 15-30 min with 1000 pixels, giving adequate time resolution to observe structures in the period of a typical magnetospheric substorm.
Akasofu Syuh-Ichi
Smith Reginald W.
Swift Daniel W.
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