The energy flux of MHD waves emerging into the solar corona

Details The energy flux of MHD waves emerging into the solar corona The energy flux of MHD waves emerging into the solar corona

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..398c&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Mar.-Apr. 1987, p. 398-404. In Russian.

Astronomy and Astrophysics

Astronomy

3

Energy Transfer, Magnetohydrodynamic Waves, Solar Corona, Field Strength, Magnetic Field Configurations, Plasma Density, Plasma Temperature, Solar Magnetic Field

Scientific paper

The propagation of MHD waves through a transition layer with a power-law profile of density and temperature is considered. The dependence of the layer transmission coefficient on the density profile and the wave frequency has been derived. It is shown that, with account for the profile, the transmission coefficient increases considerably as compared to the case of an abrupt temperature jump. Estimates of the maximum possible energy flux emerging into the corona are given which, in all practically important situations, is controlled by the value of the coronal magnetic field. The magnetic configurations are assumed to be opened ones.

Affiliated with

Also associated with

No associations

Rating

The energy flux of MHD waves emerging into the solar corona 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 energy flux of MHD waves emerging into the solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The energy flux of MHD waves emerging into the solar corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1347803