Photospheric downflows: How deep, how coherent, how important? Chapter uri icon



  • 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.

publication date

  • January 31, 1998

Date in CU Experts

  • April 13, 2014 9:41 AM

Full Author List


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