A Review of What Numerical Simulations Tell Us about the Internal Rotation of the Sun
- 1 January 1987
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Nonlinear convection of a compressible fluid in a rotating spherical shellThe Astrophysical Journal Supplement Series, 1986
- Numerical simulations of stellar convective dynamos. II - Field propagation in the convection zoneThe Astrophysical Journal, 1985
- Numerical simulations of stellar convective dynamos III. At the base of the convection zoneGeophysical & Astrophysical Fluid Dynamics, 1985
- Numerical simulations of stellar convective dynamos. I. the model and methodJournal of Computational Physics, 1984
- Internal rotation of the SunNature, 1984
- Dynamically consistent nonlinear dynamos driven by convection in a rotating spherical shell. II - Dynamos with cycles and strong feedbacksThe Astrophysical Journal Supplement Series, 1983
- Dynamically consistent nonlinear dynamos driven by convection in a rotating spherical shellThe Astrophysical Journal Supplement Series, 1981
- Compressible convection in a rotating spherical shell. I - Anelastic equations. II - A linear anelastic model. III - Analytic model for compressible vorticity wavesThe Astrophysical Journal Supplement Series, 1981
- Nonlinear dynamics of boussinesq convection in a deep rotating spherical shell-iGeophysical & Astrophysical Fluid Dynamics, 1977
- The Anelastic Approximation for Thermal ConvectionJournal of the Atmospheric Sciences, 1969