Influence of low-degree high-order p-mode splittings on the solar rotation profile

Solar Physics

Volumn 251, Issue 1-2, 2008, Pages 119-133

  Garcia R A ^a   Mathur, S ^a   Ballot, J ^b   Eff Darwich, A ^c,d   Jimenez Reyes S J ^d   Korzennik, S G ^e  

^a CEA SACLAY   (France)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c UNIVERSIDAD DE LA LAGUNA   (Spain)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Core; Helioseismology; Interior; Inverse modeling; Observations; Radiative zone; Rotation

Indexed keywords

EID: 50249105673     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-008-9144-5     Document Type: Article

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