Elementary flare bursts and eruptive plasma diagnostics

Details Elementary flare bursts and eruptive plasma diagnostics Elementary flare bursts and eruptive plasma diagnostics

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..154z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Feb. 1989, p. 154-160. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

9

Microwave Emission, Plasma Diagnostics, Solar Flares, Solar Spectra, Solar X-Rays, Chromosphere, Cosmic Rays, Dense Plasmas, Emission Spectra, High Temperature Plasmas, Magnetohydrodynamic Waves, Solar Magnetic Field

Scientific paper

The deep modulation of hard and X-ray and microwave emission of solar flares with a period of about 10 s is explained in terms of Alfvenic oscillations of a flaring loop. The oscillations are excited during the fast evaporation of the chromospheric material and the upward motion of the dense hot plasma. It is possible to estimate the density and temperature of the eruptive plasma and the mean value of the flaring loop magnetic field on the basis of the pulsation period, modulation depth, a quality of pulsation.

Affiliated with

Also associated with

No associations

Rating

Elementary flare bursts and eruptive plasma diagnostics 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 Elementary flare bursts and eruptive plasma diagnostics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elementary flare bursts and eruptive plasma diagnostics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885598