Peak asymmetry of solar p modes: A framework to explain the effects of the correlated noise from the acoustic source

Monthly Notices of the Royal Astronomical Society

Volumn 371, Issue 4, 2006, Pages 1731-1736

  Toutain, T ^a   Elsworth, Y ^a   Chaplin, W J ^a  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

Author keywords

Methods: data analysis; Methods: statistical; Sun: helioseismology

Indexed keywords

ACOUSTIC NOISE; ACOUSTICS; WHITE NOISE;

ASYMMETRIC PROFILE; BACKGROUND NOISE; CORRELATED NOISE; LORENTZIAN SHAPES; METHODS. DATA ANALYSIS; METHODS:STATISTICAL; PEAK ASYMMETRY; POWER-SPECTRA; SOLAR P MODES; SUN: HELIOSEISMOLOGY;

ACOUSTIC NOISE MEASUREMENT;

EID: 33748709653     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10798.x     Document Type: Article

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