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Data_part1: Prescribed sea ice cover of model experiments. (Data used to draw Figure 1) Data_part2: Annual mean and daily variance of surface temperature and precipitation from coupled and atmospheric model experiments. (Data used to draw Figure 3 and Figure 6) Data_part3: Temperature and precipitation extremes calculated using daily outputs of maximum and minimum surface temperature, and total precipitation from coupled and atmospheric model experiments. (Data used to draw Figure 4-5 and Figure 7-8) Data_part4: Zonal mean of zonal wind in winter and summer from coupled model experiments. (Data used to draw Figure 9) Data_part5: The seasonal average of monthly output of Sea Level Pressure, zonal wind and meridional wind in winter and summer from coupled experiments; eddy kinetic energy calculated using daily output of zonal wind and meridional wind from coupled experiments. (Data used to draw Figure 10) Data_part6: Model outputs of surface heat flux from coupled and atmospheric model experiments. (Data used to calculate northward atmospheric heat transport and draw Figure 11.) Data_part7: Temperature and precipitation extremes calculated using dynamical components of daily maximum and minimum surface temperature, and total precipitation from coupled model experiments. (Data used to draw figure 12-13.)

Data generated in this study arearchived here.

The Phanerozoic Eon has witnessed considerable changes in the climate system as well as abundant animals and plant life. Therefore, the evolution of the climate system in this Eon is worthy of extensive research. Only by studying climate changes in the past can we understand the driving mechanisms for climate changes in the future and make reliable climate projections. Apart from observational paleoclimate proxy datasets, climate simulations provide an alternative approach to investigate past climate conditions of the Earth, especially for long time span in the deep past. Here we perform 55 snapshot simulations for the past 540 million years, with a 10-million-year interval, using the Community Earth System Model version 1.2.2 (CESM1.2.2). The climate simulation dataset includes global distributions of monthly surface temperatures and precipitation, with a 1° horizontal resolution of 0.9° × 1.25° in latitude and longitude. This open access climate dataset is useful for multidisciplinary research, such as paleoclimate, geology, geochemistry, and paleontology.

Characterizing the atmospheres of extrasolar planets is the new frontier in exoplanetary science. The last two decades of exoplanet discoveries have revealed that exoplanets are very common and extremely diverse in their orbital and bulk properties. We now enter a new era as we begin to investigate the chemical diversity of exoplanets, their atmospheric and interior processes, and their formation conditions. Recent developments in the field have led to unprecedented advancements in our understanding of atmospheric chemistry of exoplanets and the implications for their formation conditions. We review these developments in the present work. We review in detail the theory of atmospheric chemistry in all classes of exoplanets discovered to date, from highly irradiated gas giants, ice giants, and super-Earths, to directly imaged giant planets at large orbital separations. We then review the observational detections of chemical species in exoplanetary atmospheres of these various types using different methods, including transit spectroscopy, Doppler spectroscopy, and direct imaging. In addition to chemical detections, we discuss the advances in determining chemical abundances in these atmospheres and how such abundances are being used to constrain exoplanetary formation conditions and migration mechanisms. Finally, we review recent theoretical work on the atmospheres of habitable exoplanets, followed by a discussion of future outlook of the field.

Eccentricity is an important orbital parameter. Understanding its effect on planetary climate and habitability is critical for us to search for a habitable world beyond our solar system. The orbital configurations of M-dwarf planets are always tidally-locked at resonance states, which are quite different from those around Sun-like stars. M-dwarf planets need to be investigated separately. Here we use a comprehensive three-dimensional atmospheric general circulation model to systematically investigate how eccentricity influences climate and habitability of M-dwarf exoplanets. The simulation results show that (1) the seasonal climatic cycles of such planets are very weak even for e = 0.4. It is unlikely that an aqua planet falls out of a habitable zone during its orbit. (2) The annual global mean surface temperature significantly increases with increased eccentricity, due to the decrease of the cloud albedo. Both the runaway greenhouse inner edge and moist greenhouse inner edge shift outward. (3) Planets in an eccentric orbit can be captured in other spin-orbit resonance states which lead to different climate patterns, namely eyeball pattern and striped-ball pattern.The striped-ball pattern has evidently higher surface temperatures due to the reduced planetary albedo. Near the outer edge, planets with p = 1.0 and 2.0 are more resistant to the snowball state due to more locally-concentrated stellar fluxes. Thus, planets with integer spin-orbit resonance numbers have wider habitable zones than those with half-integer spin-orbit resonance states. Above all, as a comparison to circular orbit, eccentricity shrinks the width of the habitable zone.

This paper summarizes the results of the researches on the middle and upper atmosphere obtained by Chinese scientists in 2008-2010. The focuses are specifically placed on the researches being associated with ground-based observation capability development, dynamical processes, the property of atmospheric circulation and the chemistry-climate coupling of the middle atmospheric layers. Keywords Middle and upper atmosphere, Metalic and airglow layer, Atmospheric tides

In this report we summarize the research results by Chinese scientists in 2012-2014. The focuses are placed on the researches of the middle and upper atmosphere, specifically the researches related to ground-based observation capability development, dynamical processes, the property of circulation and chemistry-climate coupling of the middle atmospheric layers.