Penetration and Overshooting in Turbulent Compressible Convection

By N. Brummell, T. Clune, J. Toomre. 2002

162 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/97f77d791a923300e7ef7cc4d61c42c4bccd376e

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Citations in the corpus

Thermal evolution of the core with a high thermal conductivity (2014, unknown): “Zahn, 1991; Brummell et al., 2002).”
The high conductivity of iron and thermal evolution of the Earth’s core (2013, background): “Direct numerical simulations have been developed to understand this process (e.g., Hurlburt et al., 1994; Brummell et al., 2002; Rogers et al., 2006), which partly confirmed scaling behaviors obtained earlier by Zahn (1991).”
Astrophysical magnetic fields and nonlinear dynamo theory (2004, background): “have allowed a more quantitative description of the pumping effect and the associated pump velocity 1 [332,333].”
INTERNAL GRAVITY WAVES IN MASSIVE STARS: ANGULAR MOMENTUM TRANSPORT (2013, unknown): “This rotation rate dependence was also found in Brummell et al. (2002).”
Simulations of Core Convection in Rotating A-Type Stars: Differential Rotation and Overshooting (2003, background): “…this trend is largely in keeping with nonlinear modeling of three-dimensional penetrative compressible convection in localized planar domains (see Brummell et al. 2002), which showed that a smaller filling factor for the plumes as realized in the more turbulent convection translates into a…”
Dynamo Action in the Solar Convection Zone and Tachocline: Pumping and Organization of Toroidal Fields (2006, background): “Fairly broad, low-amplitude upflows coexist with fast, concentrated downflows, which are characteristic of turbulent compressible convection (e.g., Brun & Toomre 2002; BMT04; Brummell et al. 2002).”
SIMULATION OF THE FORMATION OF A SOLAR ACTIVE REGION (2010, background): “The downward transport of such U-loops, which allows the discharge of mass from the rising magnetic field, is related to the phenomenon known as turbulent pumping (Tobias et al. 1998; Brummell et al. 2002).”
Simulations of Dynamo Action in Fully Convective Stars (2007, background): “Such coherent downflow plumes have previously been noted as a seemingly generic feature of turbulent compressible convection (e.g., Brummell et al. 2002; Brun & Toomre 2002).”