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Annual Review of Fluid Mechanics, ISSN 0066-4189, 01/2009, Volume 41, Issue 1, pp. 317 - 345
Journal Article
Solar Physics, ISSN 0038-0938, 2/2014, Volume 289, Issue 2, pp. 441 - 458
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... 
Flux emergence | Extraterrestrial Physics, Space Sciences | Global dynamo | Astrophysics and Astroparticles | Atmospheric Sciences | Convection zone | Magnetic buoyancy | Physics | FIELDS | FLUX TUBES | MODEL | HELICITY | EVOLUTION | ASTRONOMY & ASTROPHYSICS | X-RAY-EMISSION | CYCLES | STARS | TURBULENT CONVECTION | SIMULATIONS | Magnetic fields | Solar physics
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 06/2016, Volume 824, Issue 2, p. 128
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 06/2016, Volume 824, Issue 1, p. 4
Journal Article
Astrophysical Journal, ISSN 0004-637X, 10/2016, Volume 829, Issue 2, p. 92
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 6/2010, Volume 6, Issue S271, pp. 347 - 352
AbstractWe reflect upon a few of the research challenges in stellar convection and dynamo theory that are likely to be addressed in the next five or so years.... 
Sun: tachocline | Stars: massive star convection | Sun: dynamo action | Sun: near-surface shear layer | Solar physics | Astrophysics | Stars & galaxies | Boundary layer
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 04/2006, Volume 641, Issue 1 I, pp. 618 - 625
Three-dimensional simulations of solar convection in spherical shells are used to evaluate the differential rotation that results as thermal boundary... 
Convection | Sun: interior | Sun: rotation | TAYLOR-PROUDMAN BALANCE | CIRCULATION | MERIDIONAL FLOW | UPPER CONVECTION ZONE | MODEL | Sun : interior | SUN | FLUX TRANSPORT DYNAMO | convection | ASTRONOMY & ASTROPHYSICS | Sun : rotation | MAGNETIC-FIELD | TURBULENT CONVECTION | ANGULAR VELOCITY
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2019, Volume 871, Issue 2, p. 217
The dynamical origins of the Sun's tachocline and near-surface shear layer (NSSL) are still not well understood. We have attempted to self-consistently... 
convection | turbulence | Sun: Rotation | stars: Kinematics and dynamics | Sun: Interior | ROTATION | Sun: interior | ASTRONOMY & ASTROPHYSICS | MERIDIONAL FLOWS | stars: kinematics and dynamics | Sun: rotation | Physics - Solar and Stellar Astrophysics
Journal Article
Solar Physics, ISSN 0038-0938, 8/2014, Volume 289, Issue 8, pp. 2823 - 2843
Journal Article