Torsional oscillations of low mode

Details Torsional oscillations of low mode Torsional oscillations of low mode

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..221s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Feb. 1985, p. 221-228.

Physics

42

Solar Oscillations, Solar Rotation, Solar Velocity

Scientific paper

Standing wave torsional oscillations of wavenumber 1/2 and 1 hemisphere-1 are studied using an improved fit to Mount Wilson magnetograph data. These oscillations are seen to be in phase with each other and with the magnetic activity cycle, and seem best represented as a flexing of the differential rotation curve. Superposing them gives a differential rotation which at solar minimum is slightly flattened at the equator but considerably (≡5%) steepened at the poles, and also tends to produce a travelling wave with wavenumber 1 hemisphere-1 that moves from pole to equator as the cycle progresses.

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