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=1991sccha..34.1354h&link_type=abstract

Science in China, Series A, Vol. 34, No. 11, p. 1354 - 1364

Physics

Scientific paper

The data of velocity and magnetic fields in the solar photosphere (5324 Å) and the chromosphere (4861 Å) clearly show the features of tangential discontinuity of velocity in the chromosphere. The velocity fields in and near the solar active region No. 88029 by the Huairou Station have been analyzed in detail. A lot of magnetohydrodynamic discontinuous surfaces, especially the tangential discontinuities, are shown from the observations. The calculations of the thickness of discontinuous layer and the evolution time of instability agree with the observational results.

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