Polarization of solar flare hard X-rays

Details Polarization of solar flare hard X-rays Polarization of solar flare hard X-rays

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..686s&link_type=abstract

Kosmicheskie Issledovaniia, vol. 16, Sept.-Oct. 1978, p. 686-697. In Russian.

Computer Science

4

Polarimeters, Polarization (Waves), Satellite-Borne Instruments, Solar Flares, Solar X-Rays, Bremsstrahlung, Intercosmos Satellites, Oso-7, Particle Acceleration, Plasma Heating, Stellar Models

Scientific paper

The paper deals with the design and principle of polarimeters of the type employed on board the Intercosmos satellites. Polarization data obtained with these instruments are compared with data calculated on the basis of various models of a nonthermal X-ray source. It is shown that both the degree and lifetime of polarization are well described by a flare model in which the flare can be decomposed completely into a number of elementary flare bursts with no residual radiation left. (Flares of this type, observed on August 2 and 7, 1972, have been discussed by van Beek, de Faiter, and de Jager, 1976.)

Affiliated with

Also associated with

No associations

Rating

Polarization of solar flare hard X-rays 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 Polarization of solar flare hard X-rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Polarization of solar flare hard X-rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-942138