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The determination of the velocity amplitude of the total photospheric motion field
Authors:Kondrashova  N. N.  Gurtovenko  E. A.
Affiliation:1.The Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev, U.S.S.R.
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Abstract:

By the analysis of the profiles of 20 weak lines observed at five centre-to-limb positions on the solar disk, radial and tangential components of the velocity amplitude of the photospheric motion field are derived in the range of optical depth - 3.0 ? lgτ5 ? +0.5.

Keywords:
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