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  • ...es in the upper atmosphere, typically CO2. This counteracts the greenhouse effect, and moreover the broken molecules will recombine to form water-vapor cloud ...radiation]] [[image:heliosphere-weather-lanzerotti.jpg|thumb|right|200px|Effect of electromagnetic radiation]]
    14 KB (1,853 words) - 17:23, 26 février 2026
  • ...s in the upper atmosphere—typically CO2. This counteracts the greenhouse effect; furthermore, the broken molecules recombine to form water-vapor clouds tha ...c radiation]] [[image:heliosphere-weather-lanzerotti.jpg|thumb|right|200px|Effect of electromagnetic radiation]]
    15 KB (2,067 words) - 19:27, 24 février 2026
  • ...ecules of the upper atmosphere, typically CO2. This thwarts the greenhouse effect, and on the other hand, the broken molecules will recombine to form clouds ...radiations]] [[image:heliosphere-weather-lanzerotti.jpg|thumb|right|200px|Effect of electromagnetic radiations]]
    15 KB (2,133 words) - 10:59, 23 mai 2022