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  • About us
    About the Department
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  • Faculty
    Fulltime faculty
  • Research
    Research directions
    Research Highlights
    Laboratory for Climate and Ocean-Atmosphere Studies
    The joint research centre for atmospheric hydrological cycle and weather modification
    PKU AOS – Harvard EPS Climate and Environment Collaborative (CEC)
  • Education
  • Lectures
    Distinguished Lectures
  • Recruitment
中文

Research

  • Research directions
  • Research Highlights
  • Laboratory for Climate and Ocean-Atmosphere Studies
  • The joint research centre for atmospheric hydrological cycle and weather modification
  • PKU AOS – Harvard EPS Climate and Environment Collaborative (CEC)

Research

  • Research directions
  • Research Highlights
  • Laboratory for Climate and Ocean-Atmosphere Studies
  • The joint research centre for atmospheric hydrological cycle and weather modification
  • PKU AOS – Harvard EPS Climate and Environment Collaborative (CEC)
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Research Highlights

Hydrologic cycle weakening in hothouse climates

发布时间:2024-04-25
 

JIACHEN LIU 、JUN YANG *、 GANG CHEN AND YONGYUN HU


Abstract

The hydrologic cycle has wide impacts on the ocean salinity and circulation, carbon and nitrogen cycles, and the ecosystem. Under anthropogenic global warming, previous studies showed that the intensification of the hydrologic cycle is a robust feature. Whether this trend persists in hothouse climates, however, is unknown. Here, we show in climate models that mean precipitation first increases with rising surface temperature, but the precipitation trend reverses when the surface is hotter than ~320 to 330 kelvin. This nonmonotonic phenomenon is robust to the cause of warming, convection scheme, ocean dynamics, atmospheric mass, planetary rotation, gravity, and stellar spectrum. The weakening occurs because of the existence of an upper limitation of outgoing longwave emission and the continuously increasing shortwave absorption by H2O and is consistent with atmospheric dynamics featuring the strong increase of atmospheric stratification and marked reduction of convective mass flux. These results have wide implications for the climate evolutions of Earth, Venus, and potentially habitable exoplanets.



https://www.science.org/doi/10.1126/sciadv.ado2515


  

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