Distortion of the p-mode peak profiles by the solar-cycle frequency shifts: do we need to worry?

Monthly Notices of the Royal Astronomical Society

Volumn 384, Issue 4, 2008, Pages 1668-1674

  Chaplin, W J ^a   Elsworth, Y ^a   New, R ^b   Toutain, T ^a  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

Author keywords

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

Indexed keywords

UNCERTAINTY ANALYSIS;

CYCLE FREQUENCIES; DATA SET; FREQUENCY SHIFT; METHODS. DATA ANALYSIS; METHODS:STATISTICAL; P MODES; P-MODES; SOLAR CYCLE; SUN: HELIOSEISMOLOGY; UNCERTAINTY;

SOLAR ENERGY;

EID: 40249115190     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12833.x     Document Type: Article

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