Other
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsh21d..01k&link_type=abstract
American Geophysical Union, Spring Meeting 2002, abstract #SH21D-01
Other
7514 Energetic Particles (2114), 7519 Flares, 7534 Radio Emissions, 7554 X Rays, Gamma Rays, And Neutrinos
Scientific paper
Solar energetic electrons are observed to escape from the Sun into interplanetary space. However, the release machanism(s) and the involved magnetic field geometry are not well understood. In particular, it is not well understood why some solar events release energetic electrons into interplanetary and others are not. Here, radio emissions (type III bursts) and insitu observations of escaping electron beams (impulsive electron events) are compared with X-ray signatures produced by electrons moving towards the Sun. The Nancay Radio Heliograph and the WAVES experiment on WIND provide the radio observations, WIND/3DP the insitu 1-300~keV electron observations. The X-ray observations are taken by the recently launched High Energy Solar Spectroscopic Imager (HESSI). First results of this study are presented.
Klein Karsten
Krucker Sa"m
Lin Robert P.
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