Fourier versus wavelet analysis of solar diameter variability

Details Fourier versus wavelet analysis of solar diameter variability Fourier versus wavelet analysis of solar diameter variability

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...278..607v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 278, no. 2, p. 607-616

Astronomy and Astrophysics

Astrophysics

21

Fourier Analysis, Rayleigh Distribution, Solar Diameter, Wavelet Analysis, Astrolabes, Heisenberg Theory, Solar Spectra

Scientific paper

Up to now, time dependence of solar radius measurements from the CERGA astrolabe has been analyzed through spectral techniques. In the present paper, we compare results obtained in using 'wavelet' instead of Fourier transform. We show that this particular data set should better be considered as a sum of wavelets rather than a superposition of stationary oscillations.

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