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Astrobiology / Space colonization / SETI / Exoplanetology / Physical oceanography / Global climate model / Climate model / Atmosphere of Earth / Planetary habitability / Astronomy / Atmospheric sciences / Space


Role of ocean heat transport in climates of tidally locked exoplanets around M dwarf stars Yongyun Hu1 and Jun Yang Laboratory for Climate and Atmosphere–Ocean Studies, Department of Atmospheric and Oceanic Sciences, S
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Document Date: 2014-01-06 20:08:51

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File Size: 1,61 MB

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City

Washington / DC / Tucson / Inst Phys / Austin / /

Company

Spiegel / Gill AE / Yongyun Hu1 / Jun Yang Laboratory / Univ Ariz Press / Cambridge Univ Press / /

Country

United Kingdom / China / /

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Event

Environmental Issue / /

Facility

National Center / Peking University / bar of CO2 / University of Chicago / The University of Texas / /

IndustryTerm

net upward energy flux / high greenhouse-gas concentrations / energy transport / divergent atmospheric energy transport / net surface energy flux / energy-conserving thermodynamics / energy fluxes / net downward energy fluxes / /

NaturalFeature

Ocean of Earth / Earth oceans / Earth ocean / /

Organization

National Natural Science Foundation of China / Chinese Academy of Sciences / the University of Chicago / University of Texas at Austin / John Templeton Foundation / School of Physics / NASA SP / Department of Atmospheric and Oceanic Sciences / National Center for Atmospheric Research / Peking University / Beijing / /

Person

Yang Ekman / Gliese / Yang Supporting / Y. Liu / Robert E. Dickinson / R. T. Pierrehumbert / Hu Supporting / /

Position

Author / RT / Reynolds RT / /

ProvinceOrState

Texas / /

PublishedMedium

Atmospheric Research / /

Technology

radiation / thermodynamics / condensation / Simulation / /

URL

www.pnas.org/cgi/content/short/1315215111 / www.pnas.org/lookup/suppl/doi / www.pnas.org/cgi/doi/10.1073/pnas.1315215111 / /

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