Helioseismic constraints on the solar structure and the solar neutrino problem.

Details Helioseismic constraints on the solar structure and the solar neutrino problem. Helioseismic constraints on the solar structure and the solar neutrino problem.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jkps...33s.557v&link_type=abstract

Journal of the Korean Physical Society, Vol. 33, Suppl. issue, p. S557 - S559

Other

Solar Models: Internal Structure, Solar Neutrinos, Helioseismology

Scientific paper

The inversion of helioseismic modes leads to precise constraints on the internal structure of the Sun, which must be satisfied by the computed solar models. Including the element segregation which occurred in the Sun since its formation leads to solar models in much better agreement with the inversion structure than those which ignore it. However the observed lithium depletion cannot be explained without other effects like mild mixing below the convection zone, or rapid mass loss in the early stages of the solar evolution. In any case the models are not compatible with the observed neutrino fluxes. Mixing near the solar core, which has been invoked as a way of decreasing the neutrino production, can be infirmed by helioseismic results. These results are discussed and solar models close to the "Seismic Sun" are presented.

Affiliated with

Also associated with

No associations

Rating

Helioseismic constraints on the solar structure and the solar neutrino problem. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Helioseismic constraints on the solar structure and the solar neutrino problem., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Helioseismic constraints on the solar structure and the solar neutrino problem. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1294822