Modeling of type III bursts dynamic spectra

Details Modeling of type III bursts dynamic spectra Modeling of type III bursts dynamic spectra

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..222..299l&link_type=abstract

Solar Physics, v. 222, Issue 2, p. 299-310 (2004).

Physics

7

Scientific paper

The one-dimensional process of spatially limited electron stream propagation in the solar corona is simulated. It is shown that the beam instability development results either in strong relaxation in velocity space and inhibition of spatial diffusion (high-stream density) or in velocity space relaxation decrease and simultaneous growth of spatial stream length (low-stream density). Assuming a profile of background plasma density to be exponential, dynamic spectra of type III bursts are modeled, which shows that the emission source velocity is constant, and a duration of the burst emission at a given frequency reduces for high-stream densities.

Affiliated with

Also associated with

No associations

Rating

Modeling of type III bursts dynamic spectra 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 Modeling of type III bursts dynamic spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling of type III bursts dynamic spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1189679