Springer-Verlag GmbH

SCORe´96: Solar Convection and Oscillations and their Relationship

The existence of strongly convecting layers in the Sun and stars provides us with a natural laboratory for the study of dynamical processes in intensely turbulent, magnetized, rotating, radiating fluids. Helioseismology has now given us a tool to measure the detailed properties of solar convection beneath the visible Sun, and thus to test our understanding of the nature of convection and of its influence on stellar structure and the radiative magnetohydrodynamics of solar convection, presenting and incorporating the newest results from numerical hydrodynamic simulations and helioseismic observations. The contributed papers present the very latest developments in each of these fields.
Authors / Editors:
182.00 USD; 149.75 EUR; 110.50 GBP
Print ISSN:

More About This Publication »


Register here for the Springer e-mail newsletter providing you with information on the latest products in your field.

Explore the Springer eBook Collection

Customer comments

No comments were found for SCORe´96: Solar Convection and Oscillations and their Relationship. Be the first to comment!