Semiclassical analysis of stellar p modes
Abstract
We present a brief overview of our first studies in developing classical and semiclassical approximations for low-degree stellar p modes, as an alternative to the formal high-frequency asymptotic expansions used earlier. The complete account of this work can be found in Roxburgh and Vorontsov (2000, 2001).
- Publication:
-
Stellar Structure and Habitable Planet Finding
- Pub Date:
- January 2002
- Bibcode:
- 2002ESASP.485..345R
- Keywords:
-
- Waves;
- Methods: Numerical;
- Stars: Oscillations