Abstract. In this article we present our state of the art of tting helioseismic p-mode spectra. We give a step by step recipe for tting the spectra: statistics of the spectra both for spatially unresolved and resolved data, the use of Maximum Likelihood estimates, the statistics of the p-mode parameters, the use of Monte-Carlo simulation and the signicance of tted parameters. The recipe is applied to synthetic low-resolution data, similar to those of the LOI, using Monte-Carlo simulations. For such spatially resolved data, the statistics of the Fourier spectrum is as-sumed to be a multi-normal distribution; the statistics of the power spectrum is not a 2 with 2 degrees of free-dom. Results for l = 1 shows that all parameters describ-ing the...
We address the problem of line spectra detection and estimation from astrophysical data. As observat...
International audienceAcoustic rates of excitation of solar p modes can be estimated from observatio...
Publisher's version/PDFAims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stoc...
In Part I we have developed a theory for fitting p-mode Fourier spectra assuming that these spectra...
It is custom in helioseismology to assume that the power spectra of time series of solar radial ve...
This paper describes a parametric method aimed at the estimation of correlation in the excitation of...
We introduce a modified version of a standard power spectrum 'peak-bagging' technique which is desig...
A simple power law model consisting of a single spectral index, a is believed to be an adequate desc...
Aims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stochastically driven pulsa...
We present a method to reduce noise in helioseismic power spectra using a non-orthogonal wavelet tr...
We investigate the frequency dependence of the power spectral density of low-degree solar p modes by...
We report on the results of the latest solarFLAG hare-and-hounds exercise, which was concerned with ...
Context. Asteroseismology has entered a new era with the availability of continuous observations fro...
International audienceSince the asteroseismic revolution, the availability of efficient and reliable...
In order to test models of the excitation of p modes and their behavior in the visible atmosphere, w...
We address the problem of line spectra detection and estimation from astrophysical data. As observat...
International audienceAcoustic rates of excitation of solar p modes can be estimated from observatio...
Publisher's version/PDFAims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stoc...
In Part I we have developed a theory for fitting p-mode Fourier spectra assuming that these spectra...
It is custom in helioseismology to assume that the power spectra of time series of solar radial ve...
This paper describes a parametric method aimed at the estimation of correlation in the excitation of...
We introduce a modified version of a standard power spectrum 'peak-bagging' technique which is desig...
A simple power law model consisting of a single spectral index, a is believed to be an adequate desc...
Aims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stochastically driven pulsa...
We present a method to reduce noise in helioseismic power spectra using a non-orthogonal wavelet tr...
We investigate the frequency dependence of the power spectral density of low-degree solar p modes by...
We report on the results of the latest solarFLAG hare-and-hounds exercise, which was concerned with ...
Context. Asteroseismology has entered a new era with the availability of continuous observations fro...
International audienceSince the asteroseismic revolution, the availability of efficient and reliable...
In order to test models of the excitation of p modes and their behavior in the visible atmosphere, w...
We address the problem of line spectra detection and estimation from astrophysical data. As observat...
International audienceAcoustic rates of excitation of solar p modes can be estimated from observatio...
Publisher's version/PDFAims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stoc...