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Earth Science and Applications From Space: National Imperatives for the Next Decade and Beyond
Chapter 2: Solar and Stellar Convection: A Perspective for Geophysical Fluid Dynamicists
The solar tachocline and its variation
What can we learn about solar cycle mechanisms from observed velocity fields?
Effect of subsurface radial differential rotation on flux-transport solar dynamos
Instability of concentrated toroidal fields in the latitudinal differential rotation below the solar convection zone
Creation of twist at the core-convection zone interface
Angular momentum transport in the solar tachocline
Dynamics of the solar interior and the solar dynamo
Differential rotation in stars with convection zones
Global Circulation of the Sun: Where are we and where are we going?
Convective dynamos for rotating stars
Dynamos of the sun and stars, and associated convection zone dynamics
The solar dynamo: Observations and theories of solar convection, global circulation, and magnetic fields
Measurements of Pollution in the Troposphere (MOPITT) Observations from EOS/Terra
Toward Stronger Coupling Between Technical Infrastructures and Institutional Processes in Data-Intensive Science
Studies in the Atmospheric Sciences
Detection and Stochastic Modeling of Nonlinear Signatures in the Geopotential Height Field of an Atmospheric General Circulation Model
A three-dimensional simulation of ozone over the North Atlantic Ocean [presentation]
Determination of area and volume densities from UARS aerosol extinction data [presentation]

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