Low-Order p Modes From Virgo Irradiance Data

Details Low-Order p Modes From Virgo Irradiance Data Low-Order p Modes From Virgo Irradiance Data

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..200..393f&link_type=abstract

Solar Physics, v. 200, Issue 1/2, p. 393-406 (2001).

Physics

3

Scientific paper

Several candidates for low-order p modes (n <= 5) and possibly g modes were found by applying mode-detection techniques such as multivariate spectral regression analysis and time-frequency analysis to the VIRGO full-disc solar irradiance data. Three out of the candidates for low-order p modes could be confirmed by significant peaks in the un-treated power spectra in good agreement with theoretical predictions. The frequency of a fourth candidate for a low-order p mode lies some 2.8 μHz below the predicted frequency. The candidates found for g modes are less reliable, since none of them could be confirmed neither by significant peaks in the un-treated power spectra nor by the detection of multiplets.

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