Hydromagnetic structure of the chromosphere near the supergranule boundary

Details Hydromagnetic structure of the chromosphere near the supergranule boundary Hydromagnetic structure of the chromosphere near the supergranule boundary

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....53..197r&link_type=abstract

Astronomy and Astrophysics, vol. 53, no. 2, Dec. 1976, p. 197-202.

Astronomy and Astrophysics

Astrophysics

7

Chromosphere, Magnetohydrodynamic Flow, Solar Granulation, Solar Magnetic Field, Stellar Models, Supersonic Flow, Atmospheric Models, Solar Atmosphere

Scientific paper

A Bernoulli flow along magnetic lines of force and the balance of forces perpendicular to it are considered to form the hydrodynamic structure of the chromosphere near the supergranulation boundary. A preliminary supersonic flow model is constructed by use of simplifying assumptions. For this model, the effective kinetic temperature, including the contribution of waves, is required to be as high as 6500 K but may be reduced substantially by improved treatment. An explanation is given of how the magnetic field and the flow regulate themselves to give supersonic velocities and height extension in the chromosphere near the supergranulation boundary. The temperature excess and the speed of downdraft are also shown to be consistent with observations.

Affiliated with

Also associated with

No associations

Rating

Hydromagnetic structure of the chromosphere near the supergranule boundary 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 Hydromagnetic structure of the chromosphere near the supergranule boundary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydromagnetic structure of the chromosphere near the supergranule boundary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1047636