The effect of time-dependent γ-pumping on buoyant magnetic structures-Reference-Cited by-同舟云学术

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The effect of time-dependent γ-pumping on buoyant magnetic structures

Published:2018-10-26 Issue:6 Volume:112 Page:414-430
ISSN:0309-1929
Container-title:Geophysical & Astrophysical Fluid Dynamics
language:en
Short-container-title:Geophysical & Astrophysical Fluid Dynamics

Author:

Ali Abrar A.¹,Silvers Lara J.¹

Affiliation:

1. Department of Mathematics, City University of London, Northampton Square, London, UK

Funder

BIS National E-infrastructure

Science and Technology Facilities Council

STFC DiRAC Operations

Publisher

Informa UK Limited

Subject

Geochemistry and Petrology,Mechanics of Materials,Geophysics,Astronomy and Astrophysics,Computational Mechanics

Link

https://www.tandfonline.com/doi/pdf/10.1080/03091929.2018.1537396

Reference31 articles.

1. Magnetic buoyancy instabilities in the presence of magnetic flux pumping at the base of the solar convection zone

2. Magnetic structures in a dynamo simulation

3. Spatially intermittent fields in photospheric magnetoconvection

4. Dynamo Models of the Solar Cycle

5. Christensen-Dalsgaard, J. and Thompson, M., Observational results and issues concerning the tachocline. In The Solar Tachocline, edited by D.W. Hughes, R. Rosner and N.O. Weiss, pp. 53–85, 2007 (Cambridge Univ. Press: Cambridge).

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