Mathematics – Probability
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pabei..16..287g&link_type=abstract
Prog. Astron., Vol. 16, No. 4, p. 287 - 304
Mathematics
Probability
Solar Models, Solar Oscillations, Solar Neutrinos
Scientific paper
The study of solar models is the most important way to understand the global structure and properties of the Sun. Developments in solar modelling in the 1990s are reviewed. The use of the MHD and OPAL equations of states and of the OPAL opacity has moved the theoretical solar oscillation frequencies much closer to the observed values. The introduction of turbulent spectrum in the local convection theory and the 3D hydrodynamic simulation convection models have increased the knowledge of convective energy transportation, as well as its influence on the global Sun. The difference of surface helium abundance between models and inversion results has been filled by diffusion effects. Surface lithium may be depleted by turbulent diffusion or big mass loss. An astrophysical solution for the solar neutrino fluxes looks unlikely. A higher probability exists for a solution from particle physics.
Dappen Werner
Gong Zhigang
Li Yan
Peng Meixian
Yuan Yongquan
No associations
LandOfFree
Research on the solar model and oscillation in 1990s (I): progress in solar models. 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 Research on the solar model and oscillation in 1990s (I): progress in solar models., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Research on the solar model and oscillation in 1990s (I): progress in solar models. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-763981