New values of gravitational moments J2 and J4 deduced from helioseismology View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2004-08

AUTHORS

R. Mecheri, T. Abdelatif, A. Irbah, J. Provost, G. Berthomieu

ABSTRACT

By applying the theory of slowly rotating stars to the Sun, the solar quadrupole and octopole moments J2 and J4 were computed using a solar model obtained from CESAM stellar evolution code (Morel, 1997) combined with a recent model of solar differential rotation deduced from helioseismology (Corbard et al., 2002). This model takes into account a near-surface radial gradient of rotation which was inferred and quantified from MDI f-mode observations by Corbard and Thompson (2002). The effect of this observational near-surface gradient on the theoretical values of the surface parameters J2, J4 is investigated. The results show that the octopole moment J4 is much more sensitive than the quadrupole moment J2 to the subsurface radial gradient of rotation. More... »

PAGES

191-197

Identifiers

URI

http://scigraph.springernature.com/pub.10.1023/b:sola.0000043563.96766.21

DOI

http://dx.doi.org/10.1023/b:sola.0000043563.96766.21

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1020287621


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