Models of coronal hole flows

Details Models of coronal hole flows Models of coronal hole flows

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ssrv...23..159s&link_type=abstract

(COSPAR, IAU, IUGG, IUPAP, and URSI, International Symposium on Solar Terrestrial Physics, Innsbruck, Austria, May 29-June 3, 19

Physics

22

Atmospheric Models, Coronal Holes, Flow Geometry, Solar Corona, Stellar Models, Boundary Conditions, Boundary Layer Plasmas, Boundary Value Problems, Dynamic Models, Flow Distribution, Strategy

Scientific paper

Models of plasma flow in coronal holes are reviewed. These models fall into four classes: (1) radial flow on a streamline along which the divergence is assumed to vary differently than as the square of the radial distance from the sun; (2) global flow along streamlines determined in some independent manner; (3) empirical models originating in or based strongly on observation; and (4) dynamic models using magnetic and plasma boundary conditions low in the corona to find both the geometry of streamlines and the flow field. Most limitations in coronal hole flow models can be eliminated by using known numerical techniques to combine models in classes (1), (2) and (3).

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