How sensitive are rotation inversions to subtle features of the dynamo?

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 559, 2004, Pages 468-471

  Howe, R ^a   Rempel, M ^b   Christensen Dalsgaard, J ^c   Hill, F ^a   Komm, R W ^a   Schou, J ^d   Thompson, M J ^e  

^a NATIONAL SOLAR OBSERVATORY   (United States)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^c AARHUS UNIVERSITY   (Denmark)

^d STANFORD UNIVERSITY   (United States)

^e IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Sun: interior; Sun: rotation

Indexed keywords

FEEDBACK; FORCE MEASUREMENT; HEAT CONVECTION; REYNOLDS NUMBER; ROTATION; SEISMOLOGY;

CONVECTION ZONE; SIMULATED INVERSION; SUN:INTERIOR; SUN:ROTATION;

SUN;

EID: 22144494215     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (4)

1. Dikpati, M., and Charbonneau, P. A Babcock-Leighton Flux Transport Dynamo with Solar-like Differential Rotation, Astrophysical Journal, Vol. 518, 508 - 520, 1999.
2. Howe, R., Christensen-Dalsgaard, J., Hill, P., Komm, R. W., Larsen, R. M., Schou, J., Thompson, M. J., and Toomre, J. Deeply Penetrating Banded Zonal Flows in the Solar Convection Zone, Astrophysical Journal, Vol. 533, L163 - L166, 2000.
3. Kichatinov, L. L., and Rüdiger, G. Λ-effect and differential rotation in stellar convection zones, Astronomy and Astrophysics, Vol. 276, 96 - 102, 1993.
4. Spruit, H. C. Origin of the torsional oscillation pattern of solar rotation, Solar Physics, Vol. 213, 1 - 21, 2003.