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David W. Hughes

3 papers here

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author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3
ORCID 0000-0002-8004-8631

identity via Semantic Scholar / OpenAlex

most citedLarge-scale Dynamo Action Driven by Velocity Shear and Rotating Convection

68 citations · 106 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 12 cited

The effects of flux transport on interface dynamos

J. Mason, D. W. Hughes, S. M. Tobias

The operation of an interface dynamo (as has been suggested for the Sun and other stars with convective envelopes) relies crucially upon the effective transport of magnetic flux be…

astro-ph2008★ 68 cited

Large-scale Dynamo Action Driven by Velocity Shear and Rotating Convection

David W. Hughes, Michael R. E. Proctor

By incorporating a large-scale shear flow into turbulent rotating convection, we show that a sufficiently strong shear can promote dynamo action in flows that in the absence of she…

astro-ph2007★ 26 cited

The Nonlinear Evolution of Instabilities Driven by Magnetic Buoyancy: A New Mechanism for the Formation of Coherent Magnetic Structures

Evy Kersale, David W. Hughes, Steven M. Tobias

Motivated by the problem of the formation of active regions from a deep-seated solar magnetic field, we consider the nonlinear three-dimensional evolution of magnetic buoyancy inst…

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