Models of transition region and coronal plasma in solar loop structures

Details Models of transition region and coronal plasma in solar loop structures Models of transition region and coronal plasma in solar loop structures

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982saosr.392a..15r&link_type=abstract

In Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1 p 15-22 (SE

Physics

2

Coronal Loops, Plasmas (Physics), Solar Simulation, Solar Wind, Space Plasmas, Chromosphere, Extraterrestrial Radiation, Models, Solar Atmosphere, Stellar Coronas

Scientific paper

The theory of coronal loops was developed and the simple version of the theory and observations are compared. It is shown that the gross properties of the confined corona can be understood by considering simple hydrostatic equilibrium models. By observing the corona it is apparent that hydrostatic models are seriously inadequate. It is suggested that observations of intensity fluctuations, of persistent up and down flows, of relatively cool matter residing at coronal heights, of apparent spatial co-mingling of hot plasmas at quite different temperatures, need a more sophisticated modeling.

Affiliated with

Also associated with

No associations

Rating

Models of transition region and coronal plasma in solar loop structures 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 Models of transition region and coronal plasma in solar loop structures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models of transition region and coronal plasma in solar loop structures will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1648357