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One of the major concerns in climate change studies is how the thermal conditions for the living environment of human beings will change in the future. In a paper recently published in Atmospheric and Oceanic Science Letters, Prof. GAO Xuejie from the Institute of Atmospheric Physics, Chinese Academy of Sciences, and his coauthors, try to answer this question based on their recently completed and unprecedented set of high-resolution (25 km) 21st century climate change simulations. These simulations were produced using the regional climate model RegCM4, driven by four global model simulations over China—the country with the world’s largest population.

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The planets and moons of our solar system are continuously being bombarded by particles hurled away from the sun. On Earth this has hardly any effect, apart from the fascinating northern lights, because the dense atmosphere and the magnetic field of the Earth protect us from these solar wind particles. But on the Moon or on Mercury things are different: There, the uppermost layer of rock is gradually eroded by the impact of sun particles. 

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During high school, Prosper Nyovanie had to alter his daily and nightly schedules to accommodate the frequent power outages that swept cities across Zimbabwe.

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