Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987baicz..38..184h&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 38, June 1987, p. 184-189.
Astronomy and Astrophysics
Astronomy
Gyromagnetism, Solar Magnetic Field, Solar Rotation, Standing Waves, Background Radiation, Least Squares Method, Polynomials, Propagation Modes, Temporal Distribution
Scientific paper
An analysis using Gegenbauer's orthogonal polynomials revealed that changes can be observed in the differential rotation of solar background magnetic fields which are similar to those described in connection with the Doppler measurements of solar differential rotation (Snodgrass and Howard, 1985). These changes can be interpreted as manifestations of low modes of stationary torsional waves. These waves have wave numbers of 0, 1/2, and 1 on a hemisphere.
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