activity
20082026
most citedMagnetic Wreaths and Cycles in Convective Dynamos

165 citations · 406 across the 11 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2023★ 2 cited

The Puzzling Structure of Solar Convection: Window into the Dynamo

Nicholas A. Featherstone, Kyle C. Augustson, Jonathan M. Aurnou +25

The operation of the solar dynamo, with all of its remarkable spatio-temporal ordering, remains an outstanding problem of modern solar physics. A number of mechanisms that might pl…

astro-ph.SR2018★ 25 cited

Driving Solar Giant Cells through the Self-Organization of Near-Surface Plumes

Nicholas J. Nelson, Nicholas A. Featherstone, Mark S. Miesch +1

Global 3D simulations of solar giant-cell convection have provided significant insight into the processes which yield the Sun's observed differential rotation and cyclic dynamo act…

astro-ph.SR2016

2-D and 3-D Models of Convective Turbulence and Oscillations in Intermediate-Mass Main-Sequence Stars

Joyce A. Guzik, T. H. Morgan, N. J. Nelson +5

We present multidimensional modeling of convection and oscillations in main-sequence stars somewhat more massive than the Sun, using three separate approaches: 1) Using the 3-D pla…

astro-ph.SR2014★ 9 cited

Generating buoyant magnetic flux ropes in solar-like convective dynamos

Nicholas J. Nelson, Mark S. Miesch

Our Sun exhibits strong convective dynamo action which results in magnetic flux bundles emerging through the stellar surface as magnetic spots. Global-scale dynamo action is believ…

astro-ph.SR2012★ 94 cited

Buoyant Magnetic Loops Generated by Global Convective Dynamo Action

Nicholas J. Nelson, Benjamin P. Brown, A. Sacha Brun +2

Our global 3D simulations of convection and dynamo action in a Sun-like star reveal that persistent wreaths of strong magnetism can be built within the bulk of the convention zone.…

astro-ph.SR2012★ 165 cited

Magnetic Wreaths and Cycles in Convective Dynamos

Nicholas J. Nelson, Benjamin P. Brown, A. Sacha Brun +2

Solar-type stars exhibit a rich variety of magnetic activity. Seeking to explore the convective origins of this activity, we have carried out a series of global 3D magnetohydrodyna…