BOOKREVIEWS
N° R1006
Author :Friedrich Kupka , Ian W. Roxburgh ,
Kwing Lam Chan
Published in 2007 by CAMBRIDGE UNIVERSITY PRESS
Address : The Edinburgh
Building, Shaftesbury Road, Cambridge CB2 2RU, UK
Telephone : 01223
312393
Fax : 01223 315052
Internet : www.cambridge.org
ISBN : 0-521-86349-x pages 524 – hardback
Convection is ubiquitous throughout the Universe, and
during the last three decades it has become the largest factor of uncertainty
in theoretical models of stars and in the interpretation of observations on the
basis of such models. Recently, numerical simulations of convection have
dramatically improved in their potential to take into account both the large
scale properties of the flow itself and the microphysical properties of the
fluid. Observations have become accurate enough to provide stringent tests for
both numerical simulations and models of convection. IAU S239 was held to
further understanding of convection, bringing together leading researchers in solar
and stellar physics, the physics of planets, and of accretion disks. With
reviews, research contributions, and detailed recordings of plenary
discussions, this book is a valuable resource for professional astronomers and
graduate students interested in the interdisciplinary study of one of the key
physical processes in astrophysics.
• Features comprehensive review articles on the
state-of-the-art in theory, numerical simulations, and observations of
convection in astrophysical objects • Discusses convection in terrestrial
planets, gaseous giant planets such as Jupiter, stars in different evolutionary
phases, and the present view of the role of convection in accretion disks •
Shows how similar methods are applied in different fields

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