Minimum variance projection is widely used in geophysical and space plasma measurements to identify the wave propagation direction and the wavenumber of the wave fields. The advantage of the minimum variance projection is its ability to estimate the energy spectra directly in the wavenumber domain using only a limited number of spatial samplings. While the minimum variance projection is constructed for discrete signals in the data, we find that the minimum variance projection can reasonably reproduce the spectral slope of the power-law spectrum if the data represent continuous power-law signals. The spectral slope study using the minimum variance projection is tested against synthetic random data with a power-law spectrum. The meth...
A simple power law model consisting of a single spectral index, a is believed to be an adequate desc...
International audienceThis paper presents a method to estimate the continuum of a gamma rays spectru...
In this article we present our state of the art of fitting helioseismic p-mode spectra. We give a s...
Interpolation and spectral analysis of signals from finite number of samples is considered. When the...
Abstract—A signal’s spectrum is a representation of the signal in terms of elementary basis function...
International audienceThis paper presents a spectral density estimator based on a Normalized Minimum...
A proof of the pointwise convergence of the multidimensional minimum variance spectral estimator as ...
This is the first of a pair of papers which address the problem of measuring the unredshifted power ...
In many branches of science, particularly astronomy and geophysics, power spectra of the form f fi ;...
International audienceGiven the spectrogram of an unknown signal embedded in a Gaussian noise, the M...
Capon's minimum variance projection for the multi-point measurements is revisited using the method o...
We revisit a recently introduced power spectrum estimation technique based on Gibbs sampling, with t...
The variance profile is defined as the power mean of the spectral density function of a stationary s...
Abstract. In this article we present our state of the art of tting helioseismic p-mode spectra. We g...
The variance profile is defined as the power mean of the spectral density function of a stationary s...
A simple power law model consisting of a single spectral index, a is believed to be an adequate desc...
International audienceThis paper presents a method to estimate the continuum of a gamma rays spectru...
In this article we present our state of the art of fitting helioseismic p-mode spectra. We give a s...
Interpolation and spectral analysis of signals from finite number of samples is considered. When the...
Abstract—A signal’s spectrum is a representation of the signal in terms of elementary basis function...
International audienceThis paper presents a spectral density estimator based on a Normalized Minimum...
A proof of the pointwise convergence of the multidimensional minimum variance spectral estimator as ...
This is the first of a pair of papers which address the problem of measuring the unredshifted power ...
In many branches of science, particularly astronomy and geophysics, power spectra of the form f fi ;...
International audienceGiven the spectrogram of an unknown signal embedded in a Gaussian noise, the M...
Capon's minimum variance projection for the multi-point measurements is revisited using the method o...
We revisit a recently introduced power spectrum estimation technique based on Gibbs sampling, with t...
The variance profile is defined as the power mean of the spectral density function of a stationary s...
Abstract. In this article we present our state of the art of tting helioseismic p-mode spectra. We g...
The variance profile is defined as the power mean of the spectral density function of a stationary s...
A simple power law model consisting of a single spectral index, a is believed to be an adequate desc...
International audienceThis paper presents a method to estimate the continuum of a gamma rays spectru...
In this article we present our state of the art of fitting helioseismic p-mode spectra. We give a s...