A Perturbed Tri-Polytropic Model of the Sun

Details A Perturbed Tri-Polytropic Model of the Sun A Perturbed Tri-Polytropic Model of the Sun

2001-07-23

arxiv.org/abs/astro-ph/0107428v1

Astronomy and Astrophysics

Astrophysics

Submitted to IAU-Colloquium185, Radial and Nonradial pulsations as probes of stellar physics, 26-31 July 2001, Leuven, Belgium

Scientific paper

Based on the Solar Standard Model SSM of Bahcall and Pinsonneault (SSM-BP2000) we developed a solar model in hydrostatic equilibrium using three polytropes, each one associated to the nuclear, the radiative and the convective regions of the solar interior. Then, we apply small periodic and adiabatic perturbations on this tri-polytropic model in order to obtain proper frequencies and proper functions which are in the p-modes range of low order 0

Affiliated with

Also associated with

No associations

Rating

A Perturbed Tri-Polytropic Model of the Sun 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 A Perturbed Tri-Polytropic Model of the Sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Perturbed Tri-Polytropic Model of the Sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-321980