Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975kosis..13..222k&link_type=abstract
Kosmicheskie Issledovaniia, vol. 13, Mar.-Apr. 1975, p. 222-235. In Russian.
Astronomy and Astrophysics
Astronomy
5
Interplanetary Medium, Propagation Modes, Solar Electrons, Astronomical Models, Electron Energy, Lines Of Force, Magnetic Effects, Satellite Observation, Solar Flares, Time Response, Type 3 Bursts
Scientific paper
A model is proposed for the propagation of solar electrons, based on data obtained by the Prognoz satellites. These data are analyzed to determine the relationship between solar flares and bursts and increases in the intensity of solar electron fluxes. According to the proposed model, after instantaneous injection into the corona, fast electrons from a solar flare are propagated as a compact bunch inside a narrow cone of interplanetary magnetic field force lines and produce type III radio bursts in their path. A small fraction of the particles in a bunch is usually detected 60 to 100 minutes after injection of a second, slower component. This model is shown to explain previous observations of particles moving along a force line without scattering as well as the previously predicted 'cone of propagation'.
Kurt Victoria G.
Logachev Iu. I.
Pisarenko N. F.
No associations
LandOfFree
Propagation of solar electrons with energy greater than 30 keV in interplanetary space 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 solar electrons with energy greater than 30 keV in interplanetary space, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Propagation of solar electrons with energy greater than 30 keV in interplanetary space will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1521461