Coronal Linear Supra-thermal Streams
Abstract
Linear structures of the Solar Corona seen on eclipse images above active regions after the flaring activity are good candidates for being produced by primary supra-thermal streams of electrons. We propose a method to compute the Compton scattering effect applied to this case and compute the corresponding diagrams. This predicted effect will be search for on eclipse data and possibly using the SoHO Lasco coronagraph observations.
- Publication:
-
SF2A-2002: Semaine de l'Astrophysique Francaise
- Pub Date:
- June 2002
- Bibcode:
- 2002sf2a.conf..143K