Publication

2012 - Springer

Language

English

Word Count

82,000 words, Guess

Page Count

328 pages

Identifiers

  • ISBN-139789401151672
  • ISBN-109401151679
  • Better World Books9789401151672
  • Open LibraryOL37423691M

Classifications

  • LCCQB600-701

Description

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.

Subjects

Other Editions

  • SCORe '96Springer2012

Reader Reviews

No reviews yet for this book.

Be the first to share your thoughts!