The Polar Cusp pp 177-192 | Cite as
Polar Cusp Features Observed By DMSP Satellites
Abstract
Among various techniques to monitor the polar cusp region, the best available way is by using several low-altitude satellites all on the noon-midnight polar orbit to perform particle precipitation measurements. Fortunately, such an opportunity occurred in the USAF Defense Meteorological Satellite Program (DMSP). Two identical satellites had circular orbits in the noon-midnight meridian at ∼ 840 km altitude. Thus the polar cusp regions over both the northern and southern polar regions could be monitored with a temporal resolution of at least once every hour per hemisphere. In this paper, we will summarize recent findings of polar cusp characteristics and dynamics based on DMSP observations.
Keywords
Solar Wind Interplanetary Magnetic Field Electron Flux Magnetic Local Time Solar Wind DensityPreview
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