Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection

Richard J.A.M. Stevens; Jin Qiang Zhong; Herman J.H. Clercx; Roberto Verzicco; Detlef Lohse; Guenter Ahlers

doi:10.1007/978-3-642-03085-7_127

Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection

Richard J.A.M. Stevens
, Jin Qiang Zhong
, Herman J.H. Clercx
, Roberto Verzicco
, Detlef Lohse
, Guenter Ahlers

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

Abstract

For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determined by the Rayleigh : formula, and by the Prandtl number :formula. Here, is the thermal expansion coefficient, 9 the gravitational acceleration, formula the difference between the imposed temperatures nand Tt at the bottom and the top of the sample, respectively, and v and ki, the kinematic viscosity and the thermal diffusivity, respectively. The rotation rate D (given in rad/s) is used in the form of the Rossby number : formula

Original language	English
Title of host publication	Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference
Editors	B. Eckhardt
Place of Publication	Berlin
Publisher	Springer
Pages	529-532
Number of pages	4
ISBN (Print)	978-3-642-03084-0
DOIs	https://doi.org/10.1007/978-3-642-03085-7_127
Publication status	Published - 2009
Event	12th European Turbulence Conference, ETC 2009 - Marburg, Germany Duration: 7 Sept 2009 → 10 Sept 2009 Conference number: 12

Publication series

Name	Springer Proceedings in Physics
Volume	132
ISSN (Print)	0930-8989

Conference

Conference	12th European Turbulence Conference, ETC 2009
Abbreviated title	ETC 2009
Country/Territory	Germany
City	Marburg
Period	7/09/09 → 10/09/09

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10.1007/978-3-642-03085-7_127

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Stevens, R. J. A. M., Zhong, J. Q., Clercx, H. J. H., Verzicco, R., Lohse, D., & Ahlers, G. (2009). Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection. In B. Eckhardt (Ed.), Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference (pp. 529-532). (Springer Proceedings in Physics; Vol. 132). Springer. https://doi.org/10.1007/978-3-642-03085-7_127

Stevens, Richard J.A.M. ; Zhong, Jin Qiang ; Clercx, Herman J.H. et al. / Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection. Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference. editor / B. Eckhardt. Berlin : Springer, 2009. pp. 529-532 (Springer Proceedings in Physics).

@inproceedings{c30c818a848f455e84bfc8a31eb662d4,

title = "Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-B{\'e}nard convection",

abstract = "For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determined by the Rayleigh : formula, and by the Prandtl number :formula. Here, is the thermal expansion coefficient, 9 the gravitational acceleration, formula the difference between the imposed temperatures nand Tt at the bottom and the top of the sample, respectively, and v and ki, the kinematic viscosity and the thermal diffusivity, respectively. The rotation rate D (given in rad/s) is used in the form of the Rossby number : formula",

author = "Stevens, \{Richard J.A.M.\} and Zhong, \{Jin Qiang\} and Clercx, \{Herman J.H.\} and Roberto Verzicco and Detlef Lohse and Guenter Ahlers",

year = "2009",

doi = "10.1007/978-3-642-03085-7\_127",

language = "English",

isbn = "978-3-642-03084-0",

series = "Springer Proceedings in Physics",

publisher = "Springer",

pages = "529--532",

editor = "B. Eckhardt",

booktitle = "Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference",

address = "Germany",

note = "12th European Turbulence Conference, ETC 2009, ETC 2009 ; Conference date: 07-09-2009 Through 10-09-2009",

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Stevens, RJAM, Zhong, JQ, Clercx, HJH, Verzicco, R, Lohse, D & Ahlers, G 2009, Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection. in B Eckhardt (ed.), Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference. Springer Proceedings in Physics, vol. 132, Springer, Berlin, pp. 529-532, 12th European Turbulence Conference, ETC 2009, Marburg, Germany, 7/09/09. https://doi.org/10.1007/978-3-642-03085-7_127

Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection. / Stevens, Richard J.A.M.; Zhong, Jin Qiang; Clercx, Herman J.H. et al.
Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference. ed. / B. Eckhardt. Berlin: Springer, 2009. p. 529-532 (Springer Proceedings in Physics; Vol. 132).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

TY - GEN

T1 - Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection

AU - Stevens, Richard J.A.M.

AU - Zhong, Jin Qiang

AU - Clercx, Herman J.H.

AU - Verzicco, Roberto

AU - Lohse, Detlef

AU - Ahlers, Guenter

N1 - Conference code: 12

PY - 2009

Y1 - 2009

N2 - For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determined by the Rayleigh : formula, and by the Prandtl number :formula. Here, is the thermal expansion coefficient, 9 the gravitational acceleration, formula the difference between the imposed temperatures nand Tt at the bottom and the top of the sample, respectively, and v and ki, the kinematic viscosity and the thermal diffusivity, respectively. The rotation rate D (given in rad/s) is used in the form of the Rossby number : formula

AB - For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determined by the Rayleigh : formula, and by the Prandtl number :formula. Here, is the thermal expansion coefficient, 9 the gravitational acceleration, formula the difference between the imposed temperatures nand Tt at the bottom and the top of the sample, respectively, and v and ki, the kinematic viscosity and the thermal diffusivity, respectively. The rotation rate D (given in rad/s) is used in the form of the Rossby number : formula

UR - https://www.scopus.com/pages/publications/84858376120

U2 - 10.1007/978-3-642-03085-7_127

DO - 10.1007/978-3-642-03085-7_127

M3 - Conference contribution

SN - 978-3-642-03084-0

T3 - Springer Proceedings in Physics

SP - 529

EP - 532

BT - Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference

A2 - Eckhardt, B.

PB - Springer

CY - Berlin

T2 - 12th European Turbulence Conference, ETC 2009

Y2 - 7 September 2009 through 10 September 2009

ER -

Stevens RJAM, Zhong JQ, Clercx HJH, Verzicco R, Lohse D, Ahlers G. Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection. In Eckhardt B, editor, Advances in Turbulence XII - Proceedings of the 12th EUROMECH European Turbulence Conference. Berlin: Springer. 2009. p. 529-532. (Springer Proceedings in Physics). doi: 10.1007/978-3-642-03085-7_127

Prandtl-, Rayleigh-, and Rossby-number dependence of heat transport in turbulent rotating Rayleigh-Bénard convection

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