Zobrazeno 1 - 10
of 296
pro vyhledávání: '"Friedrich H. Busse"'
Publikováno v:
Fluids, Vol 6, Iss 1, p 41 (2021)
The onset of convection in the form of magneto-inertial waves in a rotating fluid sphere permeated by a constant axial electric current is studied in this paper. Thermo-inertial convection is a distinctive flow regime on the border between rotating t
Externí odkaz:
https://doaj.org/article/a4869916faaf4369862e08289688ed97
Publikováno v:
Chaos, Solitons & Fractals. 109:107-117
The analysis of the Taylor-Couette problem in the small gap limit is extended to the cases of tertiary and quaternary solutions. The theoretical results are compared with experimental observations. Although in the latter the small-gap approximation i
Autor:
Thomas Hartlep, Friedrich H. Busse
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 112:20-35
Convection in a homogeneously cooled layer heated by a fixed temperature at the lower boundary is investigated numerically for various Rayleigh numbers Ra and Prandtl numbers Pr. The upper boundary...
Autor:
Friedrich H. Busse, Ralf Kaiser
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 111:355-368
In dynamo theory the toroidal velocity theorem in its classical version (Elsasser, Phys. Rev. 1946, vol. 69, pp. 106–116, Bullard and Gellman, Phil. Trans. R. Soc. Lond. 1954, vol. A247, pp. 213–278) rules out dynamo action in a spherical conduct
Publikováno v:
European Journal of Mechanics - B/Fluids. 61:16-24
The onset of convection in a horizontal layer of an electrically conducting fluid heated from below is studied in the presence of a horizontal magnetic field rotating about a vertical axis. Two different ranges of the rotation frequency are considere
Publikováno v:
Fluids
Volume 6
Issue 1
Fluids, Vol 6, Iss 41, p 41 (2021)
Volume 6
Issue 1
Fluids, Vol 6, Iss 41, p 41 (2021)
The onset of convection in the form of magneto-inertial waves in a rotating fluid sphere permeated by a constant axial electric current is studied in this paper. Thermo-inertial convection is a distinctive flow regime on the border between rotating t
Stellar radiative zones are typically assumed to be motionless in standard models of stellar structure but there is sound theoretical and observational evidence that this cannot be the case. We investigate by direct numerical simulations a three-dime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6c6340b6ad3d826986636a22f8e8f71
The dynamics of stably stratified stellar radiative zones is of considerable interest due to the availability of increasingly detailed observations of Solar and stellar interiors. This article reports the first non-axisymmetric and time-dependent sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::501f9aa87410f269cc1dae4272b52935
Autor:
Friedrich H. Busse
Publikováno v:
European Journal of Mechanics - B/Fluids. 47:35-38
Significant effects of compression on the dynamics of convection in gases can be obtained in centrifuges. Because of the dominant role of the Coriolis force, convection in the form of propagating thermal Rossby waves will be generated at onset. At fi
Autor:
Friedrich H. Busse, Yoshi-Yuki Hayashi, Johannes Wicht, Adolfo Ribeiro, Sabine Stanley, Luis Leopoldo Silva, David Gubbins, Hiroaki Matsui, E. M. Heien, Ben Maurice Brown, Weijia Kuang, Rainer Hollerbach, Andrey Sheyko, Radostin D. Simitev, Futoshi Takahashi, Nicholas Featherstone, M. S. Avery, Bruce A. Buffett, Gary A. Glatzmaier, Christopher J. Davies, Louise H. Kellogg, Nathanaël Schaeffer, Youhei Sasaki, Thomas Gastine, Lorraine J. Hwang, Ashley P. Willis, Weiyuan Jiang, Andrew Jackson, Peter Olson, Maylis Landeau, Shin-ichi Takehiro, Jean-Luc Guermond, Jonathan M. Aurnou, Chris A. Jones, Philippe Marti, Julien Aubert, Ulrich R. Christensen
Publikováno v:
Geochemistry, Geophysics, Geosystems
Geochemistry, Geophysics, Geosystems, AGU and the Geochemical Society, 2016, 17 (5), pp.1586-1607. ⟨10.1002/2015GC006159⟩
Matsui, H; Heien, E; Aubert, J; Aurnou, JM; Avery, M; Brown, B; et al.(2016). Performance benchmarks for a next generation numerical dynamo model. Geochemistry, Geophysics, Geosystems, 17(5), 1586-1607. doi: 10.1002/2015GC006159. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/5dn9q5rf
Geochemistry Geophysics Geosystems, vol 17, iss 5
Geochemistry, Geophysics, Geosystems, vol 17, iss 5
Geochemistry, Geophysics, Geosystems, 2016, 17 (5), pp.1586-1607. ⟨10.1002/2015GC006159⟩
Geochemistry, Geophysics, Geosystems, AGU and the Geochemical Society, 2016, 17 (5), pp.1586-1607. ⟨10.1002/2015GC006159⟩
Matsui, H; Heien, E; Aubert, J; Aurnou, JM; Avery, M; Brown, B; et al.(2016). Performance benchmarks for a next generation numerical dynamo model. Geochemistry, Geophysics, Geosystems, 17(5), 1586-1607. doi: 10.1002/2015GC006159. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/5dn9q5rf
Geochemistry Geophysics Geosystems, vol 17, iss 5
Geochemistry, Geophysics, Geosystems, vol 17, iss 5
Geochemistry, Geophysics, Geosystems, 2016, 17 (5), pp.1586-1607. ⟨10.1002/2015GC006159⟩
© 2016. American Geophysical Union. All Rights Reserved. Numerical simulations of the geodynamo have successfully represented many observable characteristics of the geomagnetic field, yielding insight into the fundamental processes that generate mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f26176162cd8c54b98d69c33d0ff4716
https://hal-insu.archives-ouvertes.fr/insu-01857606/document
https://hal-insu.archives-ouvertes.fr/insu-01857606/document