LATEST SALES & OFFERS: PROMOTIONS

Close Notification

Your cart does not contain any items

Dynamics of Solar and Stellar Convection Zones and Atmospheres

IAU S365

Alexander V. Getling (Moscow State University) Leonid L. Kitchatinov (Russian Academy of Sciences, Irkutsk)

$230.95

Hardback

Not in-store but you can order this
How long will it take?

QTY:

English
Cambridge University Press
20 February 2025
Impressive events of magnetic energy release, such as solar and stellar flares and coronal mass ejections, take place in the atmospheric layers above a star's photosphere. These magnetic-activity events are closely related to the dynamics of subsurface convection zones inside the star. IAU Symposium 365 was devoted to observational and theoretical aspects of solar and stellar hydrodynamics and magnetohydrodynamics, both global and local, including numerical studies. The last few decades have been marked by substantial progress in our understanding of the physics of internal and external processes in the Sun and solar-type stars, but the scientific communities making this progress have not traditionally worked closely together. This symposium, delayed due to the COVID pandemic, brought together specialists in the physics of convection zones and atmospheres, to stimulate the emergence of new ideas and to develop new techniques in this dynamic field of active research.
Edited by:   , ,
Imprint:   Cambridge University Press
Country of Publication:   United Kingdom
Dimensions:   Height: 254mm,  Width: 178mm,  Spine: 21mm
Weight:   880g
ISBN:   9781108490771
ISBN 10:   1108490778
Series:   Proceedings of the International Astronomical Union Symposia and Colloquia
Pages:   400
Publication Date:  
Audience:   General/trade ,  ELT Advanced
Format:   Hardback
Publisher's Status:   Active

See Also