Princeton University / University of Twente / laboratory Re / Princeton Plasma Physics Laboratory / Oxford University / University of Wisconsin / 18 / New College / University of Maryland / /
IndustryTerm
gas flow / close binary star systems / online version / liquid-metal experiment / extended device / online access / energy / metal / liquid-metal system / orbital gas motion / oscillatory solutions / electricity / stable systems / disk systems / liquid metal / law acceleration / astrophysical systems / /
NaturalFeature
Cary Forest / /
Organization
Princeton University in New Jersey / US Department of Energy / National Science Foundation / University of Maryland / University of Twente in the Netherlands / New College / National Aeronautics and Space Administration / Oxford University / Royal Society / University of Wisconsin / /
Person
Mark McCaughrean / Steven Balbus / Nikolai Shakura / Günther Rüdiger / Cami Collins / Evgeny Velikhov / Maurice Couette / DANA BERRY / Hantao Ji / Rashid Sunyaev / John Hawley / Eric Edlund / Rainer Hollerbach / Elle Starkman / /
Position
Professor of Astronomy / cellent conductor / physicist / professor of astrophysical sciences / sensible viscous model for turbulent accretion disks / /
Angular momentum transport in astrophysics and in the lab Hantao Ji and Steven Balbus For evolving astrophysical accretion disks to concentrate their mass and still conserve angular momentum, turbulent flows are crucial.