Ozone Hole Affects Upper-Atmosphere Temperature and Circulation
نویسندگان
چکیده
منابع مشابه
Evaluating the performance of Atmosphere-Ocean Global Circulation Models (AOGCM) in simulating temperature variable in Ahwaz and Abadan stations
Climate changes caused by global warming has presented challenges to human society. Studying the Changes of climate variables in the future decades by using output data’s of Atmosphere-Ocean Global Circulation Models (AOGCM) is a way of perusing climate fluctuation in a region. In this study, the focus is on the AOGCM proceeds in simulating of variable temperature in Ahwaz and Abadan stations. ...
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Temperature variations of Titan’s upper atmosphere due to the plasma interaction of the satellite with Saturn’s magnetosphere and Titan’s high altitude monomer haze particles can imply an offset of up to ±30 K from currently estimated model profiles. We incorporated these temperature uncertainties as an offset into the recently published Vervack et al. (2004) (Icarus, Vol. 170, 91–112) engineer...
متن کاملMean circulation and ozone buildup
The mean meridional circulation and midlatitude ozone buildup G. Nikulin and A. Karpechko Swedish Institute of Space Physics, Atmospheric Research Programme, Box 812, SE-98112 Kiruna, Sweden Finnish Meteorological Institute, Arctic Research Centre, Tähteläntie 62, FIN-99600 Sodankylä, Finland Received: 9 May 2005 – Accepted: 26 May 2005 – Published: 30 June 2005 Correspondence to: G. Nikulin (g...
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With a detailed chemistry scheme for the middle atmosphere up to 70 km which has been added to the 3-D Karlsruhe simulation model of the middle atmosphere (KASIMA), the eects of coupling chemistry and dynamics through ozone are studied for the middle atmosphere. An uncoupled version using an ozone climatology for determining heating rates and a coupled version using on-line ozone are compared ...
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The thermal structure of the upper atmosphere of Mars has been theoretically investigated. The exospheric temperature, for a pure CO(2) model atmosphere, lies between 400 degrees and 700 degrees K. The origin of the Martian atmosphere is discussed in the light of these results.
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ژورنال
عنوان ژورنال: Asian Journal of Earth Sciences
سال: 2011
ISSN: 1819-1886
DOI: 10.3923/ajes.2011.104.104