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Titlebook: Atmospheric Ozone Dynamics; Observations in the Costas Varotsos Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 1997 Atmosph

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发表于 2025-3-21 19:14:47 | 显示全部楼层 |阅读模式
期刊全称Atmospheric Ozone Dynamics
期刊简称Observations in the
影响因子2023Costas Varotsos
视频video
学科分类Nato ASI Subseries I:
图书封面Titlebook: Atmospheric Ozone Dynamics; Observations in the  Costas Varotsos Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 1997 Atmosph
影响因子An increasing allllo~/allce because of the anthropogenically induced ozone depletion and relevant illcrca5e of the surface ultraviolet (UV) radiation (including erythemal part of the UV spectrum) has resulted in the growth of interest to total ozone (TOZ) surface and satellite observations, surface UV measurements (with an emphasis on UV -B) and. the interpretation of observation results to assess potential impacts of the UV radiation enhancement on man and biosphere. The significance of this phenomenon is diJIcrent in various cowltries. Special attention has been paid, for instance, to ozone depletion and UV radiation increase at high latitudes (this problem has also been discussed during the Workshop). It is equally clear, however, that low and mid-latitude environmental dynamics requires carefuU monitoring and assessment of environm(:ntal trends as well. Such a conclusion is especially true for the Mediterranean Region where numerous resort places are located and subject to excessive levels of Solar Ultraviolet Radiation. This is why the NATO Advanced Rcsearch Workshop "Ground-Level and Satellite Ozone Observations: Changes in the Mediterranean Region" was organized and took pla
Pindex Conference proceedings 1997
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Variations of Stratospheric Ozone at the Time of Extremely High Solar Activity,s from the modelling are: 1) 5% increase of TOC from minimum to maximum solar activity (F. 100–200) is due basically to the photochemistry; 2) At F. equal to 350, the calculated photochemical increase of TOC is about 9%; 3) In all ’diapason of data for F. (from 100 to 350) the increase of TOC follow
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AMFTRAN: A New Monte Carlo Radiative Transfer Model for Calculating Air Mass Factors,ce model, developed at the University of Bremen, Germany, within the scope of the GOME project..AMFTRAN is currently applied to perform sensitivity studies for the airmass factor under a wide range of geophysical conditions (such as viewing geometry, refraction, surface albedo, molecular absorber pr
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,Kompakte Riemann’sche Flächen,nics in Stara Zagora observatory. The main results of these investigations show that the TOC before and after the geomagnetic storm shows small variations. A 10% increase of ozone density near the maximum of the layer, in return for the tropospheric decreases was observed. A well pronounced increase
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Sätze von Bloch, Picard und Schottkyrical modeling results. A special attention has been paid to assessments of the greenhouse warming versus aerosol cooling. Then possibilities of the early detection of a greenhouse climate signal have been analysed and a few comments on the global climate observing system have been made with the gen
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https://doi.org/10.1007/978-3-540-68824-2ce model, developed at the University of Bremen, Germany, within the scope of the GOME project..AMFTRAN is currently applied to perform sensitivity studies for the airmass factor under a wide range of geophysical conditions (such as viewing geometry, refraction, surface albedo, molecular absorber pr
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Conference proceedings 1997y true for the Mediterranean Region where numerous resort places are located and subject to excessive levels of Solar Ultraviolet Radiation. This is why the NATO Advanced Rcsearch Workshop "Ground-Level and Satellite Ozone Observations: Changes in the Mediterranean Region" was organized and took pla
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