Test of the second order asymptotic theory with low degree solar gravity modes
Conference
·
OSTI ID:6643012
Further testing of first and second order asymptotic theory predictions for solar gravity modes is possible with the work of gu and Hill in which the number of classified low-degree gravity mode multiplets was increased from 31 to 53. In an extension of the work where the properties of 31 multiplets were analyzed in the framework of first order asymptotic theory, a new analysis has been performed using the properties of the 53 classified multiplets. The result of this analysis again shows the inadequacy of first order asymptotic theory for describing the eigenfrequency spectrum and clearly demonstrates the necessity of using second order asymptotic theory. 30 refs.
- Research Organization:
- Arizona Univ., Tucson (USA). Dept. of Physics
- DOE Contract Number:
- FG02-87ER13670
- OSTI ID:
- 6643012
- Report Number(s):
- CONF-8801129-1; ON: DE89003073
- Country of Publication:
- United States
- Language:
- English
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