The time delay of X-ray peak fluxes of solar flares at different energy ranges and stabilization of electron beams.

Details The time delay of X-ray peak fluxes of solar flares at different energy ranges and stabilization of electron beams. The time delay of X-ray peak fluxes of solar flares at different energy ranges and stabilization of electron beams.

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..354k&link_type=abstract

Pis'ma Astron. Zh., Tom 15, No. 4, p. 354 - 357

Astronomy and Astrophysics

Astronomy

Solar Plasma: Cerenkov Radiation, Plasma Diagnostics: Solar Flares, X Rays: Solar Flares

Scientific paper

The stability of an electron beam in solar plasma is considered. It is shown that the condition of Cherenkov resonance is fulfilled for slow non-ordinary waves for mean values of magnetic field B, plasma concentration n and mean beam velocity v ≡ 0.3 c. The stabilization of electron beam occurs due to the process of induced scattering of plasmons on thermal electrons. The stabilization occurs nonsimultaneously for electrons with various energies. Time delay estimations coincide with experimental ones.

Affiliated with

Also associated with

No associations

Rating

The time delay of X-ray peak fluxes of solar flares at different energy ranges and stabilization of electron beams. 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 The time delay of X-ray peak fluxes of solar flares at different energy ranges and stabilization of electron beams., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The time delay of X-ray peak fluxes of solar flares at different energy ranges and stabilization of electron beams. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1739627