abstract
- 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.
Photospheric downflows: How deep, how coherent, how important?
Chapter
Overview
CU Boulder Authors
publication date
- January 31, 1998
Date in CU Experts
- April 13, 2014 9:41 AM
Full Author List
- RAST MP
Full Editor List
- Christensen-Dalsgaard J; Rosenthal CS
author count
- 1
Other Profiles
International Standard Book Number (ISBN) 10
- 0792348524
International Standard Book Number (ISBN) 13
- 9780792348528