Using magnetic fluids to model convection of planetary or stellar interiors in laboratory scale-Reference-Cited by-同舟云学术

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Using magnetic fluids to model convection of planetary or stellar interiors in laboratory scale

Published:2018-12 Issue:1 Volume:18 Page:
ISSN:1617-7061
Container-title:PAMM
language:en
Short-container-title:Proc. Appl. Math. Mech.

Author:

Szabo Peter S. B.¹,Früh Wolf‐Gerrit¹

Affiliation:

1. School of Engineering and Physical ScienceHeriot‐Watt University Riccarton, Edinburgh EH14 4AS UK

Publisher

Wiley

Subject

Electrical and Electronic Engineering,Atomic and Molecular Physics, and Optics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/pamm.201800028

Reference7 articles.

1. P. SBSzabo M.BekovićandW.‐G.Früh.Using infrared thermography to investigate thermomagnetic convection under spatial non‐uniform magnetic field. IJoTS 116:118–128 2017.

2. P. SBSzaboandW.‐G.Früh.The transition from natural convection to thermomagnetic convection of a magnetic fluid in a non‐uniform magnetic field. JMMM 447:116–123 2018.

3. W.‐G.Früh.Amplitude vacillation in baroclinic flows pages 61–81. John Wiley & Sons Inc 2014.

4. W.‐G.Früh.Using magnetic fluids to simulate convection in a central force field in the laboratory. NPGPhy 12:877–889 2005.

5. F. H.Busse.Thermal instabilities in rapidly rotating systems. J. Fluid Mech. 44(3):441–460 1970.

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