Solar gravity modes - Detection and identification

Physics

Scientific paper

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Power Spectra, Solar Gravitation, Solar Oscillations, Vibration Mode, Solar Physics, Spectral Signatures

Scientific paper

Analytical methods for the detection and identification of very low frequency gravity modes in the solar oscillation are presented. The relative ease of detection of 5-min p-modes is contrasted with the difficulties posed by noisy spectra, visibility problems, complex mode signature, side lobes, and rotational splitting from g-modes. Theoretical criteria are developed and shown to permit the simultaneous detection and identification of g-modes from data of the quality presently available, and improved results are predicted if longer-time-series observations can be obtained. Graphs, digrams, and tables are provided.

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