Gravitational multipole moments of the Sun determined from helioseismic estimates of the internal structure and rotation

Details Gravitational multipole moments of the Sun determined from helioseismic estimates of the internal structure and rotation Gravitational multipole moments of the Sun determined from helioseismic estimates of the internal structure and rotation

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...377..688r&link_type=abstract

Astronomy and Astrophysics, v.377, p.688-690 (2001)

Astronomy and Astrophysics

Astrophysics

19

Rotation, Helioseismology

Scientific paper

We determine the gravitational multipole moments J2n, n=1,5, of the sun using a model of the interior structure and of solar rotation obtained from helioseismic inversions. The differential rotation of the convective zone and the underlying transition zone make only a small (~0.5%) contribution to the quadrupole moment J_2 which is found to have a value ~2.21x 10-7.

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