On comparing estimates of low-l solar p-mode frequencies from Sun-as-a-star and resolved observations

Astronomy and Astrophysics

Volumn 424, Issue 2, 2004, Pages 713-717

  Chaplin, W J ^a   Appourchaux, T ^b,d   Elsworth, Y ^a   Isaak, G R ^a   Miller, B A ^a   New, R ^c  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b EUROPEAN SPACE AGENCY   (Netherlands)

^c SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

^d UNIVERSITÉ PARIS SUD   (France)

Author keywords

Methods: data analysis; Sun: helioseismology

Indexed keywords

ASTRONOMICAL SATELLITES; DATA REDUCTION; HARMONIC ANALYSIS; IMAGE ANALYSIS; IMAGING SYSTEMS; POLYNOMIALS; SEISMOLOGY; SOLAR RADIATION; SUN;

IMAGE DECOMPOSITION; SOLAR CYCLES; SUN: HELIOSEISMOLOGY;

ASTROPHYSICS;

EID: 4544252838     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040501     Document Type: Article

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