A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 2, 2011, Pages 1158-1174

  Christensen Dalsgaard, J ^a,b   Monteiro, M J P F G ^c,d   Rempel, M ^b   Thompson, M J ^b,e  

^a AARHUS UNIVERSITY   (Denmark)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^c CENTRO DE ASTROFÍSICA   (Portugal)

^d UNIVERSITY OF PORTO   (Portugal)

^e UNIVERSITY OF SHEFFIELD   (United Kingdom)

Author keywords

Asteroseismology; Convection; Stars: interiors; Sun: helioseismology; Sun: interior

Indexed keywords

ASTEROSEISMOLOGY; CONVECTION; CONVECTIVE ENVELOPE; ELEMENT DIFFUSION; HELIOSEISMOLOGY; SOLAR DYNAMO; STANDARD SOLAR MODELS; STARS: INTERIORS; SUN: HELIOSEISMOLOGY; SUN: INTERIOR;

ASTROPHYSICS;

EID: 79958157759     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18460.x     Document Type: Article

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