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Science requirements of the COSMO K-Coronagraph
Technical Report: Survey of cyberinfrastructure needs and interests of NSF-funded principal investigators
Conceptual design of the COSMO K-coronagraph
Chromatic aberration in a singlet coronagraph objective lens
Measurement Error in the COSMO K-Coronagraph
How close are we to the two degree limit?
Global sources of local pollution: An assessment of long-range transport of key air pollutants to and from the United States
Household survey data used in calibrating the Population-Environment-Technology Model
Production data for the population-environment-technology (PET) model
Low-energy astrophysics: Stimulating the reduction of energy consumption in the next decade
Magnetically driven activity in the solar corona: A path to understanding the energetics of astrophysical plasmas
Causes of solar activity
Solar dynamo and magnetic self-organization
Temporal variability of stars and stellar systems
Magnetic flux emergence on the Sun and Sun-like stars
Dynamos and magnetic fields of the Sun and other cool stars, and their role in the formation and evolution of stars and in the habitability of planets
Sampling physical ocean fields in WCRP CMIP5 simulations: CLIVAR Working Group on Ocean Model Development (WGOMD) committee on CMIP5 ocean model output
Is the climate sensitivity even more uncertain?
Evaluating global warming potentials with historical temperature: An application of ACC2 inversion
Report of the U.S. CLIVAR Salinity Science Working Group

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