Observation of solar low-l p-modes by the CORONAS-DIFOS experiment.

Details Observation of solar low-l p-modes by the CORONAS-DIFOS experiment. Observation of solar low-l p-modes by the CORONAS-DIFOS experiment.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...322l..41h&link_type=abstract

Astronomy and Astrophysics, v.322, p.L41-L44

Astronomy and Astrophysics

Astrophysics

5

Sun: Oscillations, Instrumentation: Photometers, Methods: Data Analysis

Scientific paper

The CORONAS satellite, launched on 1994 March 2, carried the DIFOS experiment to observe irradiance fluctuations due to global solar oscillations. The DIFOS experiment was working for almost 50-days near solar activity minimum. We present first results of the Fourier analysis of the full time series. The fine structure of the low-l p-modes is shown and fitted with Lorentzian line profiles. Results of the wavelet analysis show strong variations of the p-modes in time.

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