Physics
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348...97j&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 97-99
Physics
1
Coronagraphs, Plasma Acceleration, Soho Mission, Solar Corona, Solar Corpuscular Radiation, Solar Wind, Computerized Simulation, Mathematical Models, Position (Location), Solar Physics
Scientific paper
The SOHO (Solar and Heliospheric Observatory) coronagraphs will offer an unprecedented opportunity to observe coronal streamer material and determine its outward motion. The inner C1 and C2 coronagraphs should enable ready identification of coronal streamers and their surface manifestations. The outer C3 coronagraph should be able to trace streamers to nearly interplanetary distances from the Sun. Using a modeling program designed to determine parameters from co-rotating heliospheric material viewed by the Helios spacecraft, the locations in position angle and distance from the Sun of several modeled streamers are shown. These models demonstrate the expected differences in streamer location when different assumptions are used for the outward acceleration of the streamer material.
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