Novel techniques for the identification of noise contributions to full-disc helioseismic power spectra
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Novel techniques for the identification of noise contributions to full-disc helioseismic power spectra. / Chaplin, W. J.; Elsworth, Y.; Isaak, G. R. et al.
SOHO 14/GONG 2004 Workshop - Helio- and Asteroseismology: Towards a Golden Future. 559. ed. 2004. p. 360-363 (European Space Agency, (Special Publication) ESA SP).Research output: Chapter in Book/Report/Conference proceeding › Conference Proceeding (Non-Journal item)
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TY - GEN
T1 - Novel techniques for the identification of noise contributions to full-disc helioseismic power spectra
AU - Chaplin, W. J.
AU - Elsworth, Y.
AU - Isaak, G. R.
AU - Miller, B. A.
AU - New, R.
AU - Pinter, B.
N1 - Copyright: Copyright 2008 Elsevier B.V., All rights reserved.
PY - 2004
Y1 - 2004
N2 - The continuum spectrum of noise found in the power spectra of Doppler shift measurements of the Sun provides information concerning non-oscillatory effects in the photosphere and forms a background against which oscillation modes must be detected. A proper determination of the continuum spectrum requires the genuine solar signal to be identified from amongst a number of instrumental effects. A number of authors have used cross-spectra form from simultaneous data sets to help to achieve such identification. In this paper we build on recent advances in the understanding of the noise characteristics of resonant scattering spectrometers to develop alternative techniques for isolating and evaluating solar and different instrumental noise contributions. Brief analyses of simulated data and BiSON measurements are presented to illustrate the potential of the techniques. helioseismology; noise level.
AB - The continuum spectrum of noise found in the power spectra of Doppler shift measurements of the Sun provides information concerning non-oscillatory effects in the photosphere and forms a background against which oscillation modes must be detected. A proper determination of the continuum spectrum requires the genuine solar signal to be identified from amongst a number of instrumental effects. A number of authors have used cross-spectra form from simultaneous data sets to help to achieve such identification. In this paper we build on recent advances in the understanding of the noise characteristics of resonant scattering spectrometers to develop alternative techniques for isolating and evaluating solar and different instrumental noise contributions. Brief analyses of simulated data and BiSON measurements are presented to illustrate the potential of the techniques. helioseismology; noise level.
UR - http://www.scopus.com/inward/record.url?scp=22144471247&partnerID=8YFLogxK
M3 - Conference Proceeding (Non-Journal item)
AN - SCOPUS:22144471247
T3 - European Space Agency, (Special Publication) ESA SP
SP - 360
EP - 363
BT - SOHO 14/GONG 2004 Workshop - Helio- and Asteroseismology:
T2 - SOHO 14/GONG 2004 Workshop - Helio- and Asteroseismology: Towards a Golden Future
Y2 - 12 July 2004 through 16 July 2004
ER -