Solar oblateness induced by its differential rotation

Details Solar oblateness induced by its differential rotation Solar oblateness induced by its differential rotation

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....14676m&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #14676

Computer Science

Scientific paper

By using the theory of Solar gravitational figure, the solar quadrupole moment J2 was computed combined with a recent analytical model of differential solar rotation (Corbard et al. 2002) taking into account a near-surface radial gradient of rotation inferred and quantified from MDI f-modes observations. This value of J2 obtained permits to evaluate the solar oblateness and its induced latitudinal variation of solar diameter. This variation was compared to those obtained from observations.

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