Formation of solar-wind energy and mass fluxes in a model with a wave source

Details Formation of solar-wind energy and mass fluxes in a model with a wave source Formation of solar-wind energy and mass fluxes in a model with a wave source

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..705c&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Sept.-Oct. 1987, p. 705-711. In Russian.

Physics

8

Energy Dissipation, Magnetohydrodynamic Waves, Mass Flow Rate, Solar Corona, Solar Wind, Stellar Models, Plasma Heating, Solar Magnetic Field, Solar Physics

Scientific paper

A self-consistent problem of corona and solar-wind formation in a spherically symmetric model with an MHD-wave energy source is examined. It is shown that the unique free parameter determining the structure of the solution is the induction of the coronal magnetic field B(asterisk). When B(asterisk) is greater than about 2 G, the outflow of matter has a significant effect on the coronal conditions. The corona parameters and solar-wind energy and mass fluxes are analyzed as a function of the B(asterisk) magnitude.

Affiliated with

Also associated with

No associations

Rating

Formation of solar-wind energy and mass fluxes in a model with a wave source 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 Formation of solar-wind energy and mass fluxes in a model with a wave source, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of solar-wind energy and mass fluxes in a model with a wave source will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1774261