Home > CSC-OpenAccess Library > Manuscript Information
EXPLORE PUBLICATIONS BY COUNTRIES |
EUROPE | |
MIDDLE EAST | |
ASIA | |
AFRICA | |
............................. | |
United States of America | |
United Kingdom | |
Canada | |
Australia | |
Italy | |
France | |
Brazil | |
Germany | |
Malaysia | |
Turkey | |
China | |
Taiwan | |
Japan | |
Saudi Arabia | |
Jordan | |
Egypt | |
United Arab Emirates | |
India | |
Nigeria |
A New Enhanced Method of Non Parametric power spectrum Estimation.
K.Suresh Reddy, S.Venkata Chalam, B.C.Jinaga
Pages - 38 - 53 | Revised - 22-02-2010 | Published - 08-04-2010
Published in Signal Processing: An International Journal (SPIJ)
MORE INFORMATION
KEYWORDS
A Nonuniform sampled data, , least-squares method, iterative adaptive approach,, periodogram,
ABSTRACT
The spectral analysis of non uniform sampled data sequences using Fourier Periodogram method is the classical approach. In view of data fitting and computational standpoints why the Least squares periodogram(LSP) method is preferable than the “classical” Fourier periodogram and as well as to the frequently-used form of LSP due to Lomb and Scargle is explained. Then a new method of spectral analysis of nonuniform data sequences can be interpreted as an iteratively weighted LSP that makes use of a data-dependent weighting matrix built from the most recent spectral estimate. It is iterative and it makes use of an adaptive (i.e., data-dependent) weighting, we refer to it as the iterative adaptive approach (IAA).LSP and IAA are nonparametric methods that can be used for the spectral analysis of general data sequences with both continuous and discrete spectra. However, they are most suitable for data sequences with discrete spectra (i.e., sinusoidal data), which is the case we emphasize in this paper. Of the existing methods for nonuniform sinusoidal data, Welch, MUSIC and ESPRIT methods appear to be the closest in spirit to the IAA proposed here. Indeed, all these methods make use of the estimated covariance matrix that is computed in the first iteration of IAA from LSP. MUSIC and ESPRIT, on the other hand, are parametric methods that require a guess of the number of sinusoidal components present in the data, otherwise they cannot be used; furthermore.
1 | Sridhar, B., & Tadisetty, S. (2015, June). ERLS non parametric spectrum sensing for CR. In Advance Computing Conference (IACC), 2015 IEEE International (pp. 185-190). IEEE. |
1 | Google Scholar |
2 | Academic Index |
3 | CiteSeerX |
4 | refSeek |
5 | iSEEK |
6 | Socol@r |
7 | Bielefeld Academic Search Engine (BASE) |
8 | Scribd |
9 | SlideShare |
10 | PDFCAST |
11 | PdfSR |
12 | Search-Docs |
B. Priestley, Spectral Analysis and Time Series, Volume 1: Univariate Series, New York: Academic, 1981. | |
E. S. Saunders, T. Naylor, and A. Allan, “Optimal placement of a limited number of observations for period searches,” Astron. Astrophys.,vol. 455, pp. 757–763, May 2006. | |
F. A. M. Frescura, C. A. Engelbrecht, and B. S. Frank, “Significance tests for periodogram peaks,” NASA Astrophysics Data System, Jun. 2007 | |
F.J.M.Barning,“The numerical analysis of the light-curve of12 lacerate,” Bull.Astronomy. Inst Netherlands, vol. 17, no. 1, pp. 22–28, Aug. 1963. | |
J. A. Fessler and B. P. Sutton, “Nonuniform fast Fourier transforms using min-max interpolation,” IEEE Trans. Signal Process., vol. 51, no. 2, pp. 560–574, Feb. 2003. | |
J. D. Scargle, “Studies in astronomical time series analysis. II—Statis- tical aspects of spectral analysis of unevenly spaced data,” Astrophys. J., vol. 263, pp 835–853, Dec. 1982. | |
J. Li and P. Stoica, “An adaptive filtering approach to spectral estimation and SAR imaging,”Trans., vol. 44, no. 6,pp. 1469–1484, Jun. 1996. | |
L. Eyer and P. Bartholdi, “Variable stars: Which Nyquist frequency?,”Astron. Astrophys. Supp Series, vol. 135, pp. 1–3, Feb. 1999. | |
N. Nguyen and Q. Liu, “The regular Fourier matrices and nonuniform fast Fourier transforms,” SIAM J. Sci. Comput., vol. 21, no. 1,pp. 283–293, 2000. | |
N. R. Lomb, “Least-squares frequency analysis of unequally spaced data,” Astrophysics . Space Sci., vol. 39, no. 2, pp. 447–462, Feb. 1976. | |
Oppenheim, A.V., and R.W. Schafer, Discrete-Time Signal Processing, Prentice-Hall, 1989, pp. 730- 742. | |
P. Reegen, “SigSpec—I. Frequency- and phase resolved significance in Fourier space,” Astron Astrophys., vol. 467, pp. 1353–1371, Mar.2007. | |
P. Stoica and R. L. Moses, Spectral Analysis of Signals Upper Saddle River, NJ: Prentice-Hall, 2005. | |
P. Stoica and Y. Selen, “Model-order selection: A review of information criterion rules,” IEEE Signal Process. Mag., vol. 21, no. 4, pp.36–47, Jul. 2004. | |
P. Vanicek, “Approximate spectral analysis by least-squares fit,” Astro- phys. Space Sci., vol. 4, no. 4, pp. 387–391, Aug. 1969. | |
P. Vanicek, “Further development and properties of the spectral anal- ysis by least- squares,” Astrophys. Space Sci.vol. 12, no. 1, pp. 10–33, Jul. 1971. | |
S. Ferraz-Mello, “Estimation of periods from unequally spaced obser- vations,” Astronom. J., vol.86, no.4, pp. 619–624, Apr. 1981. | |
Stoica,P and R.L. Moses, Introduction to Spectral Analysis, Prentice-Hall, 1997, pp. 24-26. | |
T. Yardibi, M. Xue, J. Li, P. Stoica, and A. B.Baggeroer, “Iterative adaptive approach for sparse signal representation with sensing applications,” IEEE Trans. Aerosp. Electron . Syst., 2007. | |
W. H. Press and G. B. Rybicki, “Fast algorithm for spectral analysis of unevenly sampled data,” Astrophys. J., vol. 338, pp. 277–280, Mar.1989. | |
Welch, P.D, "The Use of Fast Fourier Transform for the Estimation of Power Spectra: A Method Based on Time Averaging Over Short, Modified Periodogram," IEEE Trans. Audio electro acoustics, Vol. AU-15 (June 1967), pp. 70-73. | |
Dr. K.Suresh Reddy
- India
Dr. S.Venkata Chalam
- India
Dr. B.C.Jinaga
- India
|
|
|
|
View all special issues >> | |
|
|