Changes in convective properties over the solar cycle: Effect on p-mode damping rates

Monthly Notices of the Royal Astronomical Society

Volumn 327, Issue 2, 2001, Pages 483-487

  Houdek, G ^a   Chaplin, W J ^b,c   Appourchaux, T ^c   Christensen Dalsgaard, J ^d,e   Dappen W ^a,f   Elsworth, Y ^b   Gough, D O ^a,g   Isaak, G R ^b   New, R ^h   Rabello Soares, M C ^d  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^c EUROPEAN SPACE AGENCY   (Netherlands)

^d THEORETICAL ASTROPHYSICS CENTER   (Denmark)

^e AARHUS UNIVERSITY   (Denmark)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^h SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

Author keywords

Convection; Sun: activity; Sun: granulation; Sun: oscillations

Indexed keywords

GRANULATION; SOLAR ENERGY; SOLAR RADIATION;

CONVECTION; CONVECTIVE PROPERTIES; FREQUENCY CHANGES; LENGTH SCALE; MAGNETIC-FIELD; P MODES; P-MODES; SUN: ACTIVITY; SUN: GRANULATION; SUN: OSCILLATIONS;

MAGNETIC FIELDS;

EID: 17044454360     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04749.x     Document Type: Article

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