The tangential discontinuous surface of velocity in solar chromosphere

Details The tangential discontinuous surface of velocity in solar chromosphere The tangential discontinuous surface of velocity in solar chromosphere

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991scsmp..34.1354h&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 1001-6511), vol. 34, no. 11, p. 13

Mathematics

Logic

Chromosphere, Magnetohydrodynamic Flow, Photosphere, Solar Magnetic Field, Solar Velocity, Velocity Distribution, Boundary Layers, Magnetic Flux, Mass Flow, Visual Observation

Scientific paper

The data of velocity and magnetic fields in the solar photosphere (5324 A) and the chromosphere (4861 A) clearly show the features of tangential discontinuity of velocity in the chromosphere. The velocity fields in and near the solar active region named No. 88029 by the Huairou Station were analyzed in detail. Many magnetohydrodynamic discontinuous surfaces, especially the tangential discontinuities, were found. Calculations of the thickness of discontinuous layer and the evolution time of instability agree with the observational results. The variations of the flowfield will directly influence the evolution and changes of the active region as the magnetic field is coupled with the plasma motion.

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