activity
20002017
most citedThe Role of Magnetic Helicity Transport in Nonlinear Galactic Dynamos

82 citations · 756 across the 32 of their papers we have counts for

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16 papers · 1 filter

astro-ph2008★ 44 cited

Turbulent dynamos in spherical shell segments of varying geometrical extent

Dhrubaditya Mitra, Reza Tavakol, Axel Brandenburg +1

We use three-dimensional direct numerical simulations of the helically forced magnetohydrodynamic equations in spherical shell segments in order to study the effects of changes in…

astro-ph2008

General Flattened Jaffe Models for Galaxies

Zhenglu Jiang, Daoyuan Fang, Hongxia Liu +1

In this paper we extend oblate and prolate Jaffe models into more general flattened Jaffe models. Since dynamical properties of oblate and prolate Jaffe Models have been studied by…

astro-ph2008★ 1 cited

Axisymmetric models for galaxies by equipotential and equidensity methods

Zhenglu Jiang, Daoyuan Fang, David Moss

In this paper we outline equipotential and equidensity methods of constructing axisymmetric models for galaxies. The former method defines equipotentials, from which the correspond…

astro-ph2006★ 28 cited

The distribution of current helicity at the solar surface at the beginning of the solar cycle

D. Sokoloff, S. D. Bao, N. Kleeorin +5

A fraction of solar active regions are observed to have current helicity of a sign that contradicts the polarity law for magnetic helicity; this law corresponds to the well-known H…

astro-ph2005★ 61 cited

The Radial Distribution of Magnetic Helicity in the Solar Convective Zone: Observations and Dynamo Theory

H. Zhang, D. Sokoloff, I. Rogachevskii +4

We continue our attempt to connect observational data on current helicity in solar active regions with solar dynamo models. In addition to our previous results about temporal and l…

astro-ph2003★ 38 cited

The influence of density stratification and multiple nonlinearities on solar torsional oscillations

Eurico Covas, David Moss, Reza Tavakol

Analyses of recent helioseismic data have produced ample evidence for substantial dynamical variation of the differential rotation within the solar convection zone. Given the inevi…