Steady flows in solar magnetic structures - a class of exact MHD solutions.

Details Steady flows in solar magnetic structures - a class of exact MHD solutions. Steady flows in solar magnetic structures - a class of exact MHD solutions.

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991gapfd..59..253d&link_type=abstract

Geophysical and Astrophysical Fluid Dynamics, Vol. 59, No. 1-4, p. 253 - 265

Physics

Fluid Dynamics

5

Solar Magnetic Fields: Structure, Magnetic Fields: Solar Corona

Scientific paper

A class of exact solutions to the steady, two-dimensional magnetohydrodynamic equations in a cylindrical geometry is presented. These may model both closed and open magnetic structures found in the solar atmosphere. For closed structures, it is found that increasing the flow speed causes the summit of the arcade of closed magnetic fieldlines to rise. Parameter ranges also exist where the solution has regions of open and closed field, and so the solutions may be relevant for modelling flows in solar magnetic structures such as coronal streamers, X-ray bright points, coronal plumes and coronal holes.

Affiliated with

Also associated with

No associations

Rating

Steady flows in solar magnetic structures - a class of exact MHD solutions. 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 Steady flows in solar magnetic structures - a class of exact MHD solutions., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Steady flows in solar magnetic structures - a class of exact MHD solutions. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1717263