Jane Pratt

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Adjunct Professor

University of Georgia

United States

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About

Jane Pratt is an Adjunct Professor at Georgia State University in the United States. Her research areas focus on the interior dynamics of stars, particularly convection and mixing processes as illustrated in her recent articles. Notable topics include convective shells in Cepheid variable stars, internal gravity waves, and hydrodynamic simulations of stellar interiors. She employs advanced numerical simulations to explore complex phenomena in stellar astrophysics.

Recent Grants

Grant: Close

Formulating a theoretical scaling for dispersion in MHD turbulence

Open Date: 2022-06-15

Close Date: 2025-05-31

Grant: Close

Statistics of Turbulent Convection

Open Date: 2019-09-01

Close Date: 2023-08-01

Grant: Close

Modernization of an advanced parallel code for high-resolution simulation of astrophysical turbulence

Open Date: 2019-09-01

Close Date: 2020-08-01

Grant: Close

CDS&E: Feedback of energetic particles on plasma turbulence

Open Date: 2019-07-15

Close Date: 2023-06-30

Grant: Close

Theoretical asteroseismology of solar-like stars

Open Date: 2018-07-01

Close Date: 2019-06-01

Articles (13)

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2025

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2025

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2024

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2024

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2023

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2023

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2022

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2022

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2022

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2022

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2020

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2020

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2020

Collaborators (3)

Angela Busse

Professor of Fluid Dynamics

University of Glasgow

UNITED KINGDOM

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Simon Campbell

MONASH UNIVERSITY

AUSTRALIA

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Adrien Morison

University of Glasgow

UNITED KINGDOM

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Jane Pratt

Research Interests

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About

Recent Grants

Articles (13)

Convective shells in the interior of Cepheid variable stars: Overshooting models based on hydrodynamic simulations

Mixing by internal gravity waves in stars: assessing numerical simulations against theory

The shape of convection in 2D and 3D global simulations of stellar interiors

Effects of stratification on overshooting and waves atop the convective core of M⊙ main-sequence stars

Two-dimensional simulations of internal gravity waves in a 5 M⊙ zero-age-main-sequence model

A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations

Reynolds number dependence of Lagrangian dispersion in direct numerical simulations of anisotropic magnetohydrodynamic turbulence

Impact of radial truncation on global 2D hydrodynamic simulations for a Sun-like model

Two-dimensional simulations of solar-like models with artificially enhanced luminosity

Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes

Lagrangian Statistics for Dispersion in Magnetohydrodynamic Turbulence

Lagrangian Statistics of Heat Transfer in Homogeneous Turbulence Driven by Boussinesq Convection

Comparison of 2D and 3D compressible convection in a pre-main sequence star

Collaborators (3)

Angela Busse

Simon Campbell

Adrien Morison

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