Time/frequency analysis of solar p-modes

Details Time/frequency analysis of solar p-modes Time/frequency analysis of solar p-modes

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...285l..29b&link_type=abstract

Astronomy and Astrophysics 285L, 29-32 (1994)

Astronomy and Astrophysics

Astrophysics

24

Methods: Data Analysis, Sun: Oscillations

Scientific paper

A time/frequency analysis method is applied firstly to simulated solar data in order to demonstrate its suitability for the analysis of solar p-modes. It is then applied to real data, using the 6 months uninterrupted set of luminosity measurements from IPHIR, which is particularly suited on account of its continuity. The method yields very interesting results: strong short-term variations of energy in individual modes, independent behaviour of the modes and of the components of a single mode. The information provided by this method is relevant to the understanding of the mechanisms which drive solar p-modes.

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