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  • 1
    Publication Date: 2019-07-13
    Description: The equatorial rotation rate of the photosphere was measured at effect data. It was found that scattered light has a large influence and must be taken into account properly. When this was done it was found that the rotation rate from Doppler shifts agreed very well with the rate found for sunspots. Short-term fluctuations in rotation rate (i.e. from day to day) were less than plus or minus 15 m/s and were thus within observational errors.
    Keywords: GEOPHYSICS
    Type: NASA-CR-157923 , SU-IPR-766 , Workshop on Solar Rotation Catania; Sep 26, 1978 - Sep 28, 1978; Sicily; Italy
    Format: application/pdf
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