F
Friedrich H. Busse
Researcher at University of Bayreuth
Publications - 371
Citations - 16920
Friedrich H. Busse is an academic researcher from University of Bayreuth. The author has contributed to research in topics: Convection & Rayleigh number. The author has an hindex of 69, co-authored 371 publications receiving 16275 citations. Previous affiliations of Friedrich H. Busse include University of California & Max Planck Society.
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Asymptotic solutions of convection in rapidly rotating non-slip spheres
TL;DR: In this paper, the authors derived asymptotic solutions describing the onset of convection in rotating, self-gravitating Boussinesq fluid spheres with no-slip boundary conditions.
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A spherical shell numerical dynamo benchmark with pseudo-vacuum magnetic boundary conditions
Andrew Jackson,Andrey Sheyko,Philippe Marti,Andreas Tilgner,David Cébron,Stijn Vantieghem,Radostin D. Simitev,Radostin D. Simitev,Radostin D. Simitev,Friedrich H. Busse,Friedrich H. Busse,X. Zhan,Gerald Schubert,Shin-ichi Takehiro,Youhei Sasaki,Yoshi-Yuki Hayashi,Adolfo Ribeiro,Caroline Nore,Caroline Nore,Jean-Luc Guermond +19 more
TL;DR: In this article, the authors compare numerical results of several different types of computer codes that are capable of solving the equations of momentum transfer, magnetic field generation and heat transfer in the setting of a spherical shell, namely a sphere containing an inner core.
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Transitions to complex flows in the Ekman–Couette layer
TL;DR: In this paper, the secondary and tertiary states of fluid flow in a layer between two plates in relative motion and rotating about a normal axis of rotation are studied numerically for a wide range of parameters.
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Large Wavelength Convection Rolls in Low Prandtl Number Fluids
TL;DR: In this article, a new instability called the skewed varicose instability was found, which causes an increase of the wavelength of convection rolls with increasing Rayleigh number. But this instability was only applied to low Prandtl number fluids.
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Generation of magnetic fields by convection in a rotating sphere, I
P. G. Cuong,Friedrich H. Busse +1 more
TL;DR: In this paper, the magnetohydrodynamic dynamo problem for an electrically conducting spherical fluid shell with spherically symmetric distributions of gravity and heat sources is solved and the dynamics of motions generated by thermal buoyancy are dominated by the effects of rotation of the fluid shell.