The relationship between meridional drift and rotation of the large-scale solar magnetic field

Details The relationship between meridional drift and rotation of the large-scale solar magnetic field The relationship between meridional drift and rotation of the large-scale solar magnetic field

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..146..401l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 146, no. 2, p. 401-404.

Physics

7

Drift, Meridional Flow, Solar Magnetic Field, Solar Rotation, Correlation Coefficients, Magnetic Signatures, Solar Physics

Scientific paper

The pattern of torsional oscillations was detected in the rotation of the large-scale magnetic field using the method of two-dimensional correlation functions. The position of areas of fast and slow rotation agrees with the Doppler picture obtained by Ulrich et al. (1988). The torsional wave amplitude is 20-40 m/s and increases with latitude. A strong correlation of the pattern of residual E-W rate with the meridional drift pattern, obtained from the same data, was determined. The sign of correlation is consistent with the results reported by Ward (1965).

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