Stability of the low degree five minute solar oscillations
Conference
·
OSTI ID:5426307
In this paper we discuss the decay rate for many of the low degree p modes observed as 5 minute oscillations of the sun. This report is an expanded version of the presentation at Snowmass. These theoretical results use the completely nonadiabatic linear theory of Saio and Cox (1980). Our solar model is based on the evolution results of Christensen-Dalsbgaard (1982). Equation of state and opacity data come from the Los Alamos Opacity Library of Huebner, Merts, Magee, and Argo (1977). We compute rates for modes ranging from radial (l = 0) to the nonradial ones with l = 5 for overtones 10 through 28.
- Research Organization:
- Los Alamos National Lab., NM (USA)
- DOE Contract Number:
- W-7405-ENG-36
- OSTI ID:
- 5426307
- Report Number(s):
- LA-UR-83-3217; CONF-8308136-2; ON: DE84003786
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
DATA
DENSITY
INFORMATION
LUMINOSITY
MAIN SEQUENCE STARS
MASS
MATHEMATICAL MODELS
NUMERICAL DATA
OPTICAL PROPERTIES
OSCILLATION MODES
OSCILLATIONS
PHYSICAL PROPERTIES
SIZE
STAR MODELS
STARS
SUN
THEORETICAL DATA
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
DATA
DENSITY
INFORMATION
LUMINOSITY
MAIN SEQUENCE STARS
MASS
MATHEMATICAL MODELS
NUMERICAL DATA
OPTICAL PROPERTIES
OSCILLATION MODES
OSCILLATIONS
PHYSICAL PROPERTIES
SIZE
STAR MODELS
STARS
SUN
THEORETICAL DATA