A two-component model of impulsive microwave burst emission consistent with soft and hard X-rays

Details A two-component model of impulsive microwave burst emission consistent with soft and hard X-rays A two-component model of impulsive microwave burst emission consistent with soft and hard X-rays

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...53..139b&link_type=abstract

Solar Physics, vol. 53, July 1977, p. 139-155.

Physics

22

Astronomical Models, Microwave Emission, Solar Radio Bursts, Solar X-Rays, Radiant Flux Density, Radiative Transfer, Solar Magnetic Field, Synchrotron Radiation

Scientific paper

A model accounting for both solar microwave flux spectra and hard and soft X-ray emission data is described. The model, which relies on a core-halo structure and an artificial representation of the magnetic field, is used in applying the full energy distribution function derived from soft and hard X-ray emission data to microwave bursts. The proposed mechanism largely replaces the effect of nonthermal gyro-resonance absorption and emission in the halo; an inhomogeneous density distribution and a generalized treatment of radiation transfer are also invoked. Data from Solrad satellites 9 and 10 are examined in light of the model.

Affiliated with

Also associated with

No associations

Rating

A two-component model of impulsive microwave burst emission consistent with soft and 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 A two-component model of impulsive microwave burst emission consistent with soft and hard X-rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A two-component model of impulsive microwave burst emission consistent with soft and hard X-rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1562074