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

Christensen-Dalsgaard, J., Monteiro, M.J.P.F.G., Rempel, M. et al. (1 more author) (2011) 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, 414 (2). pp. 1158-1174. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • Christensen-Dalsgaard, J.
  • Monteiro, M.J.P.F.G.
  • Rempel, M.
  • Thompson, M.J.
Copyright, Publisher and Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2011 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: asteroseismology; convection; Sun: helioseismology; Sun: interior; stars: interiors; OSCILLATION FREQUENCIES; PENETRATIVE CONVECTION; SCALING RELATIONSHIPS; SOUND-SPEED; ZONE; SUN; HELIUM; DIFFUSION; BOTTOM; MODELS
Dates:
  • Published: June 2011
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 06 Nov 2017 10:39
Last Modified: 06 Nov 2017 10:39
Published Version: https://doi.org/10.1111/j.1365-2966.2011.18460.x
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1111/j.1365-2966.2011.18460.x

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