A new efficient method for determining weighted power spectra: Detection of low-frequency solar p-modes by analysis of BiSON data

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 2, 2011, Pages 1310-1321

  Fletcher, S T ^a   Broomhall, A M ^b   Chaplin, W J ^b   Elsworth, Y ^b   New, R ^a  

^a SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF BIRMINGHAM   (United Kingdom)

Author keywords

Methods: data analysis; Sun: helioseismology; Sun: oscillations

Indexed keywords

COMPUTATIONAL EFFICIENCY; FAST FOURIER TRANSFORMS; FOURIER SERIES;

BIRMINGHAM; DATA SET; METHODS. DATA ANALYSIS; NEW EFFICIENT METHOD; POWER-SPECTRA; SOLAR OSCILLATIONS; SOLAR P MODES; SUN: HELIOSEISMOLOGY; SUN: OSCILLATIONS; WEIGHTED POWER;

POWER SPECTRUM;

EID: 79960570277     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18779.x     Document Type: Article

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