Extension of range in radial order in detection and mode classification of solar low-degree gravity modes

Details Extension of range in radial order in detection and mode classification of solar low-degree gravity modes Extension of range in radial order in detection and mode classification of solar low-degree gravity modes

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990scsmp..33..854h&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 1001-6511), vol. 33, July 1990, p.

Mathematics

Logic

4

Solar Gravitation, Solar Interior, Solar Oscillations, Fourier Transformation, Particle Interactions, Particle Mass, Stellar Structure, Weak Interactions (Field Theory)

Scientific paper

Differential radius observations of the sun obtained in the SCLERA program (Bos and Hill, 1983) during 1979 are analyzed for evidence of detectable solar g-modes, beyond that presented by Hill (1985). The procedures and criteria employed are explained, and the results are presented in graphs. The number of g-mode multiplets identified on the basis of statistically significant evidence and classified is extended from the 31 of Hill (1985) to 53, and the degrees and radial orders of all the multiplets are listed.

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