Hydrostatic and dynamic models of solar coronal holes

Details Hydrostatic and dynamic models of solar coronal holes Hydrostatic and dynamic models of solar coronal holes

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...216..141r&link_type=abstract

Astrophysical Journal, Part 1, vol. 216, Aug. 15, 1977, p. 141-157. Research supported by the Smithsonian Institution;

Astronomy and Astrophysics

Astrophysics

44

Dynamic Models, Magnetohydrostatics, Solar Atmosphere, Solar Corona, Solar Wind, Stellar Models, Atmospheric Models, Chromosphere, Energy Transfer, Far Ultraviolet Radiation, Heat Flux, Magnetohydrodynamic Flow, One Dimensional Flow, Radio Spectra, Steady Flow, X Ray Spectra

Scientific paper

A description is presented of a sequence of one-dimensional fluid flow models of the transition zone and the inner corona. A hydrostatic model atmosphere in reasonable agreement with observations of closed, large-scale coronal structures found in the quiet sun is considered and various physical effects are introduced, one at a time, observing the response of the model. As a result of the investigations, a model is developed of the plasma flow in a coronal hole. It is shown that the data severely circumscribe the allowable range of possible models.

Affiliated with

Also associated with

No associations

Rating

Hydrostatic and dynamic models of solar coronal holes 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 Hydrostatic and dynamic models of solar coronal holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydrostatic and dynamic models of solar coronal holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1880249