Search Results - "Browning, Matthew K."

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  1. 1

    Magnetism, dynamo action and the solar-stellar connection by Brun, Allan Sacha, Browning, Matthew K.

    Published in Living reviews in solar physics (2017)
    “…The Sun and other stars are magnetic: magnetism pervades their interiors and affects their evolution in a variety of ways. In the Sun, both the fields…”
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  2. 2

    Magnetic Cycles in a Convective Dynamo Simulation of a Young Solar-type Star by Brown, Benjamin P, Miesch, Mark S, Browning, Matthew K, Brun, Allan Sacha, Toomre, Juri

    Published in The Astrophysical journal (10-04-2011)
    “…Young solar-type stars rotate rapidly and many are magnetically active. Some appear to undergo magnetic cycles similar to the 22 yr solar activity cycle. We…”
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  3. 3

    Persistent Magnetic Wreaths in a Rapidly Rotating Sun by Brown, Benjamin P, Browning, Matthew K, Brun, Allan Sacha, Miesch, Mark S, Toomre, Juri

    Published in The Astrophysical journal (01-03-2010)
    “…When our Sun was young it rotated much more rapidly than now. Observations of young, rapidly rotating stars indicate that many possess substantial magnetic…”
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  4. 4

    Helicity inversion in spherical convection as a means for equatorward dynamo wave propagation by Duarte, Lúcia D. V., Wicht, Johannes, Browning, Matthew K., Gastine, Thomas

    “…We discuss here a purely hydrodynamical mechanism to invert the sign of the kinetic helicity, which plays a key role in determining the direction of…”
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  5. 5

    Dynamo Action in the Solar Convection Zone and Tachocline: Pumping and Organization of Toroidal Fields by Browning, Matthew K, Miesch, Mark S, Brun, Allan Sacha, Toomre, Juri

    Published in The Astrophysical journal (10-09-2006)
    “…We present the first results from three-dimensional spherical shell simulations of magnetic dynamo action realized by turbulent convection penetrating downward…”
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  6. 6

    Simulations of Core Convection in Rotating A-Type Stars: Magnetic Dynamo Action by Brun, Allan Sacha, Browning, Matthew K, Toomre, Juri

    Published in The Astrophysical journal (10-08-2005)
    “…Core convection and dynamo activity deep within rotating A-type stars of 2 M sub( )are studied with three-dimensional nonlinear simulations. Our modeling…”
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  7. 7

    Simulations of Dynamo Action in Fully Convective Stars by Browning, Matthew K

    Published in The Astrophysical journal (01-04-2008)
    “…We present three-dimensional nonlinear magnetohydrodynamic simulations of the interiors of fully convective M dwarfs. Our models consider 0.3 solar- mass stars…”
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  8. 8

    Convection with misaligned gravity and rotation: simulations and rotating mixing length theory by Currie, Laura K, Barker, Adrian J, Lithwick, Yoram, Browning, Matthew K

    “…ABSTRACT We present numerical simulations, using two complementary set-ups, of rotating Boussinesq thermal convection in a three-dimensional Cartesian geometry…”
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  9. 9

    The Radius and Entropy of a Magnetized, Rotating, Fully Convective Star: Analysis with Depth-dependent Mixing Length Theories by Ireland, Lewis G., Browning, Matthew K.

    Published in The Astrophysical journal (01-04-2018)
    “…Some low-mass stars appear to have larger radii than predicted by standard 1D structure models; prior work has suggested that inefficient convective heat…”
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  10. 10

    Simulations of Solar and Stellar Dynamos and Their Theoretical Interpretation by Käpylä, Petri J., Browning, Matthew K., Brun, Allan Sacha, Guerrero, Gustavo, Warnecke, Jörn

    Published in Space science reviews (01-10-2023)
    “…We review the state of the art of three dimensional numerical simulations of solar and stellar dynamos. We summarize fundamental constraints of numerical…”
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  11. 11

    Viscous dissipation and dynamics in simulations of rotating, stratified plane-layer convection by Lance, Simon R W, Currie, Laura K, Browning, Matthew K

    “…ABSTRACT Convection in stars and planets must be maintained against viscous and Ohmic dissipation. Here, we present the first systematic investigation of…”
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  12. 12

    THEORETICAL LIMITS ON MAGNETIC FIELD STRENGTHS IN LOW-MASS STARS by Browning, Matthew K., Weber, Maria A., Chabrier, Gilles, Massey, Angela P.

    Published in The Astrophysical journal (20-02-2016)
    “…ABSTRACT Observations have suggested that some low-mass stars have larger radii than predicted by 1D structure models. Some theoretical models have invoked…”
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  13. 13

    MODELING THE RISE OF FIBRIL MAGNETIC FIELDS IN FULLY CONVECTIVE STARS by Weber, Maria A., Browning, Matthew K.

    Published in The Astrophysical journal (20-08-2016)
    “…ABSTRACT Many fully convective stars exhibit a wide variety of surface magnetism, including starspots and chromospheric activity. The manner by which bundles…”
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  14. 14

    Effects of Fossil Magnetic Fields on Convective Core Dynamos in A-type Stars by Featherstone, Nicholas A, Browning, Matthew K, Brun, Allan Sacha, Toomre, Juri

    Published in The Astrophysical journal (01-11-2009)
    “…The vigorous magnetic dynamo action achieved within the convective cores of A-type stars may be influenced by fossil magnetic fields within their radiative…”
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  15. 15

    Rapidly Rotating Suns and Active Nests of Convection by Brown, Benjamin P, Browning, Matthew K, Brun, Allan Sacha, Miesch, Mark S, Toomre, Juri

    Published in The Astrophysical journal (20-12-2008)
    “…In the solar convection zone, rotation couples with intensely turbulent convection to drive a strong differential rotation and achieve complex magnetic dynamo…”
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  16. 16

    Simulations of Core Convection in Rotating A-Type Stars: Differential Rotation and Overshooting by Browning, Matthew K, Brun, Allan Sacha, Toomre, Juri

    Published in The Astrophysical journal (20-01-2004)
    “…We present the results of three-dimensional simulations of core convection within A-type stars of 2 M sub(o), at a range of rotation rates. We consider the…”
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    Viscous Dissipation and Dynamics in Simulations of Rotating, Stratified Plane-layer Convection by Lance, Simon R. W, Currie, Laura K, Browning, Matthew K

    Published 22-01-2024
    “…Convection in stars and planets must be maintained against viscous and Ohmic dissipation. Here, we present the first systematic investigation of viscous…”
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