Solar p-mode frequencies at ℓ = 2: What do analyses of unresolved observations actually measure?

Astronomy and Astrophysics

Volumn 416, Issue 1, 2004, Pages 341-351

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

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b EUROPEAN SPACE AGENCY   (Netherlands)

^c SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

^d UNIVERSITÉ CÔTE D'AZUR   (France)

^e UNIVERSITY OF OSLO   (Norway)

Author keywords

Methods: data analysis; Sun: helioseismology; Sun: magnetic fields

Indexed keywords

COMPUTER SIMULATION; DOPPLER EFFECT; MAGNETIC FIELDS; SATELLITES; SPACECRAFT OBSERVATORIES; SUN;

HELIOSEISMOLOGY; SOLAR MODE FREQUENCIES;

ASTRONOMY;

EID: 1542646361     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034465     Document Type: Article

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