Opacity Determination in the Solar Radiative Interior

Details Opacity Determination in the Solar Radiative Interior Opacity Determination in the Solar Radiative Interior

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.277.1567e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 277, NO. 4/DEC15, P.1567, 1995

Astronomy and Astrophysics

Astronomy

7

Sun: Abundances - Sun: Interior - Sun: Oscillations

Scientific paper

Kernels are developed which express the sensitivity of solar acoustic oscillation frequencies to changes in opacity at fixed radius. Inversion is carried out using the method of optimally localized averaging to obtain linear combinations of frequency differences between the real Sun and a reference model which represent localized averages of the opacity difference between the two. Reference models are constructed with and without helium settling and inversions are carried out relative to these models. No evidence is found for helium or heavy element settling.

Affiliated with

Also associated with

No associations

Rating

Opacity Determination in the Solar Radiative Interior 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 Opacity Determination in the Solar Radiative Interior, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Opacity Determination in the Solar Radiative Interior will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1562426