Solar-cycle related variation of solar differential rotation
arXiv:1305.4174 · doi:10.1093/mnras/stt744
Abstract
Solar-cycle related variation of differential rotation is investigated through analyzing the rotation rates of magnetic fields, distributed along latitudes and varying with time at the time interval of August 1976 to April 2008. More pronounced differentiation of rotation rates is found to appear at the ascending part of a Schwabe cycle than at the descending part on an average. The coefficient in the standard form of differential rotation, which represents the latitudinal gradient of rotation, may be divided into three parts within a Schwabe cycle. Part one spans from the start to the year of a Schwabe cycle, within which the absolute is approximately a constant or slightly fluctuates. Part two spans from the to the year, within which the absolute decreases. Part three spans from the year to the end, within which the absolute increases. Strong magnetic fields repress differentiation of rotation rates, so that rotation rates show less pronounced differentiation, but weak magnetic fields seem to just reflect differentiation of rotation rates. The solar-cycle related variation of solar differential rotation is inferred to the result of both the latitudinal migration of the surface torsional pattern and the repression of strong magnetic activity to differentiation of rotation rates.
19 pages, 8 figures, accepted by MNRAS. arXiv admin note: text overlap with arXiv:1305.3970
References in corpus (6)
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Cited by in corpus (5)
- Measurements of Solar Differential Rotation Using the Century Long Kodaikanal Sunspot Data
- The rotation rate of solar active and ephemeral regions -- I. Dependence on morphology and peak magnetic flux
- Large-scale photospheric motions determined from granule tracking and helioseismology from SDO/HMI data
- The Extended Solar Cycle and Asymmetry of the Large-Scale Magnetic Field
- Hemispheric asymmetry in the sunspot cycle as a nonextensive phenomenon