Exploitation of Space Data for Innovative Helio- and Asteroseismology

    Helioseismology











    Power spectrum

    power spectrum

    This package contains code to
    1) compute an azimuthally averaged power spectrum and
    2) fit the spectrum at constant wave number as a function of frequency (some Model S efrequencies to use as a guess) and return the fit parameters. The fitting function fits asymmetric Lorentzians to each peak and returns the parameters of the Lorentzian for each peak.

     

    Downloads:
    The code uses the IDL MPFIT fitting library .

    The package is pow_spectra.tar.gz

    If you use these programs please contact schunker [at] mps.mpg.de for the appropriate acknowledgements.

     

     

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