Solar wind - The quasi-radial approximation and its limitations

Details Solar wind - The quasi-radial approximation and its limitations Solar wind - The quasi-radial approximation and its limitations

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...40..487s&link_type=abstract

Solar Physics, vol. 40, Feb. 1975, p. 487-499.

Physics

14

Astronomical Models, Interplanetary Magnetic Fields, Perturbation Theory, Radial Flow, Solar Wind Velocity, Approximation, Axisymmetric Flow, Inertial Reference Systems, Magnetic Effects, Partial Differential Equations, Pressure Distribution, Radial Velocity, Solar Corona, Solar Magnetic Field

Scientific paper

The mathematical basis for approximating the solar wind expansion as nearly radial is examined and defined, removing earlier restrictions thought to occur in the presence of a magnetic field and large variations in latitude. The equations and side conditions governing quasi-radial flow are derived and solved for a simple example to illustrate how this technique can be used for global models of the solar wind.

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