Numerical modeling of the solar tachocline. I. Freely evolving stratified turbulence in a thin rotating spherical shell

Astrophysical Journal

Volumn 562, Issue 2 PART II, 2001, Pages 1058-1075

  Miesch, Mark S ^a,b  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

Sun: interior; Sun: rotation; Turbulence

Indexed keywords

EID: 0001317861     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/323527     Document Type: Article

References (5)

1. Abramowitz, M., & Stegun, I. A. 1965, Handbook of Mathematical Functions (New York: Dover)
2. Basu, S. 1997, MNRAS, 288, 572
3. Brun, A. S., & Toomre, J. 2001, ApJ, submitted
4. Charbonneau, P., Christensen-Dalsgaard, J., Henning, R., Larsen, R. M., Schou, J., Thompson, M. J., & Tomczyk, S. 1999a, ApJ, 527, 445
5. Charbonneau, P., Dikpati, M., & Gilman, P. A. 1999b, ApJ, 526, 523