Semiclassical approximation for low-degree stellar p modes - II. Classical ray tracing

Monthly Notices of the Royal Astronomical Society

Volumn 317, Issue 1, 2000, Pages 151-157

  Roxburgh, I W ^a   Vorontsov, S V ^b  

^a OBSERVATOIRE DE PARIS   (France)

^b SCHMIDT INSTITUTE OF PHYSICS OF THE EARTH   (Russian Federation)

Author keywords

Methods: numerical; Stars: oscillations; Waves

Indexed keywords

NUMERICAL METHODS; STARS;

ACOUSTICS WAVES; LOW DEGREE; METHOD: NUMERICAL; MODE II; RAY-TRACING TECHNIQUE; SEMI-CLASSICAL APPROXIMATION; SEMICLASSICAL APPROXIMATIONS; STAR OSCILLATIONS; STELLAR INTERIOR; STELLAR P-MODES;

RAY TRACING;

EID: 0000499915     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03624.x     Document Type: Article

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