Crossref Citations
This article has been cited by the following publications. This list is generated based on data provided by
Crossref.
Kerswell, R.R.
1997.
Variational bounds on shear-driven turbulence and turbulent Boussinesq convection.
Physica D: Nonlinear Phenomena,
Vol. 100,
Issue. 3-4,
p.
355.
Doering, Charles R.
and
Hyman, James M.
1997.
Energy stability bounds on convective heat transport:mNumerical study.
Physical Review E,
Vol. 55,
Issue. 6,
p.
7775.
Kerswell, Richard R.
and
Malkus, Willem V. R.
1998.
Tidal instability as the source for Io's magnetic signature.
Geophysical Research Letters,
Vol. 25,
Issue. 5,
p.
603.
Fearn, D R
1998.
Hydromagnetic flow in planetary cores.
Reports on Progress in Physics,
Vol. 61,
Issue. 3,
p.
175.
Doering, C. R.
1999.
Fundamental Problematic Issues in Turbulence.
p.
3.
Kerswell, R. R.
1999.
Variational principle for the Navier-Stokes equations.
Physical Review E,
Vol. 59,
Issue. 5,
p.
5482.
Zhang, Keke
and
Schubert, Gerald
2000.
Magnetohydrodynamics in Rapidly Rotating spherical Systems.
Annual Review of Fluid Mechanics,
Vol. 32,
Issue. 1,
p.
409.
Wang, Xiaoming
2000.
Effect of tangential derivative in the boundary layer on time averaged energy dissipation rate.
Physica D: Nonlinear Phenomena,
Vol. 144,
Issue. 1-2,
p.
142.
Vanyo, J. P.
and
Dunn, J. R.
2000.
Core precession: flow structures and energy.
Geophysical Journal International,
Vol. 142,
Issue. 2,
p.
409.
Buffett, Bruce A.
2000.
Earth's Deep Interior: Mineral Physics and Tomography From the Atomic to the Global Scale.
Vol. 117,
Issue. ,
p.
37.
Vitanov, Nikolay K.
2000.
Upper bounds on convective heat transport in a rotating fluid layer of infinite Prandtl number: Case of intermediate Taylor numbers.
Physical Review E,
Vol. 62,
Issue. 3,
p.
3581.
Vitanov, Nikolay K.
2003.
Convective heat transport in a rotating fluid layer of infinite Prandtl number: Optimum fields and upper bounds on Nusselt number.
Physical Review E,
Vol. 67,
Issue. 2,
Shalimov, S. L.
2006.
On the precession driven geodynamo.
Izvestiya, Physics of the Solid Earth,
Vol. 42,
Issue. 6,
p.
460.
Dehant, V.
Lammer, H.
Kulikov, Y. N.
Grießmeier, J.-M.
Breuer, D.
Verhoeven, O.
Karatekin, Ö.
Van Hoolst, T.
Korablev, O.
and
Lognonné, P.
2007.
Planetary Magnetic Dynamo Effect on Atmospheric Protection of Early Earth and Mars.
Space Science Reviews,
Vol. 129,
Issue. 1-3,
p.
279.
Dehant, V.
Lammer, H.
Kulikov, Y. N.
Grießmeier, J. -M.
Breuer, D.
Verhoeven, O.
Karatekin, Ö.
Van Hoolst, T.
Korablev, O.
and
Lognonné, P.
2007.
Geology and Habitability of Terrestrial Planets.
Vol. 24,
Issue. ,
p.
279.
Wu, Cheng Chin
and
Roberts, Paul H.
2008.
A precessionally-driven dynamo in a plane layer.
Geophysical & Astrophysical Fluid Dynamics,
Vol. 102,
Issue. 1,
p.
1.
Xuan, Chuang
and
Channell, James E.T.
2008.
Origin of orbital periods in the sedimentary relative paleointensity records.
Physics of the Earth and Planetary Interiors,
Vol. 169,
Issue. 1-4,
p.
140.
Wu, Cheng-Chin
and
Roberts, Paul H.
2009.
On a dynamo driven by topographic precession.
Geophysical & Astrophysical Fluid Dynamics,
Vol. 103,
Issue. 6,
p.
467.
Vitanov, N. K.
2010.
Optimum fields and bounds on heat transport for nonlinear convection in rapidly rotating fluid layer.
The European Physical Journal B,
Vol. 73,
Issue. 2,
p.
265.
Le Bars, M.
Lacaze, L.
Le Dizès, S.
Le Gal, P.
and
Rieutord, M.
2010.
Tidal instability in stellar and planetary binary systems.
Physics of the Earth and Planetary Interiors,
Vol. 178,
Issue. 1-2,
p.
48.