Diffusional component of nonrelativistic solar electrons

Details Diffusional component of nonrelativistic solar electrons Diffusional component of nonrelativistic solar electrons

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18.1010k&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 18, Nov.-Dec. 1978, p. 1010-1016. In Russian.

Computer Science

Electron Diffusion, Nonrelativistic Mechanics, Solar Electrons, Diffusion Coefficient, Electron Energy, Electron Flux Density, Interplanetary Magnetic Fields, Solar Wind, Time Dependence

Scientific paper

A function approximating the diffusional time profiles of the intensity of 21 increases of solar electrons with energies exceeding 30 keV and 40 keV, respectively, is presented. It is shown that the slow component of the increases is described well by the simple diffusion equation. Electron diffusion coefficients for the 30-40 keV range lie within the range 8 x 10 to the 20th sq cm/sec to 1.2 x 10 to the 22nd sq cm/sec; changes of the diffusion coefficient are related to changes in the number of particles injected in the event. For the slow component, scattering of electrons takes precedence over the collimating effect of the interplanetary magnetic field.

Affiliated with

Also associated with

No associations

Rating

Diffusional component of nonrelativistic solar electrons 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 Diffusional component of nonrelativistic solar electrons, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diffusional component of nonrelativistic solar electrons will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-887133