Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007a%26a...463.1143o&link_type=abstract
Astronomy and Astrophysics, Volume 463, Issue 3, March I 2007, pp.1143-1152
Astronomy and Astrophysics
Astrophysics
1
Sun: Particle Emission, Sun: Flares, Sun: Magnetic Fields, Sun: Atmosphere, X-Rays: Bursts, Sun: Radio Radiation
Scientific paper
Aims:The electron transport is investigated numerically after an electron transport model is deduced. Methods: This model for electron propagation considers global electric and magnetic fields, as well as local Coulomb collisions. A new way to handle the electron's pitch angle evolution by using a binary dice within the treatment of the Coulomb scattering is introduced. The conditions in the solar plasma are represented by average and commonly used models, such that numerical simulations can be performed easily. Results: The model for electron propagation finally obtained makes it possible to investigate how the Coulomb collisions act on the pitch angle, while electrons are transported through the solar plasma. Some chosen numerical results for different initial conditions are presented in the paper.
Mann Gottfried
Önel Hakan
Sedlmayr Erwin
No associations
LandOfFree
Propagation of energetic electrons through the solar corona and the interplanetary medium does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Propagation of energetic electrons through the solar corona and the interplanetary medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Propagation of energetic electrons through the solar corona and the interplanetary medium will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-856583