Tracing the streamer belt through the interplanetary medium

Details Tracing the streamer belt through the interplanetary medium Tracing the streamer belt through the interplanetary medium

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...91b&link_type=abstract

Observatoire de Paris-Meudon, International Solar Wind 8 Conference, p. 91

Astronomy and Astrophysics

Astronomy

Interplanetary Medium, Interplanetary Space, Solar Activity Effects, Solar Wind, Energetic Particles, Radio Emission, Solar Rotation, International Sun Earth Explorer 3, Solar Wind Velocity, Sun, Satellite Observation

Scientific paper

Storms of mildly energetic electrons, continuously ejected from solar active regions produce long lasting radio emissions which can be traced over periods of days as the Sun rotates. They are the radio trace large scale regions expanding through interplanetary space and closely associated with helmet streamer structures. They are a common phenomena during the period of solar maximum. The solar wind velocity in these structures can be obtained up to about 0.5 Astronomical Unit. they are almost always associated with slow solar wind. We review and discuss observations of ISEE-3 in the context of our present knowledge of the solar wind structure.

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