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Free access article

Issue A&A
Volume 377, Number 2, October II 2001
Page(s) 688 - 690
Section The Sun
DOI http://dx.doi.org/10.1051/0004-6361:20011104



A&A 377, 688-690 (2001)
DOI: 10.1051/0004-6361:20011104

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

I. W. Roxburgh

Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK LESIA, Observatoire de Paris, Place Jules Janssen, 92155 Meudon, France

(Received 12 July 2001 / Accepted 31 July 2001 )

Abstract
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 ($\approx$ $0.5\%$) contribution to the quadrupole moment J2 which is found to have a value $\approx$ $2.21\times 10^{-7}$.


Key words: rotation -- helioseismology




© ESO 2001

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