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dc.contributor.authorMöser, Werner
dc.contributor.authorRaschke, Ehrhard
dc.date.accessioned2017-06-09T13:59:57Z
dc.date.available2017-06-09T13:59:57Z
dc.date.copyright1984/01/01
dc.date.issued1984
dc.identifier.issn0733-3021
dc.identifier.otherams-10651.pdf
dc.identifier.urihttp://onlinelibrary.yabesh.ir/handle/yetl/4145792
dc.description.abstractDaily sums of the downward solar radiation, i.e., the global radiation, have been computed from imaging data of reflected solar and emitted infrared radiation which were measured from the geostationary satellites METEOSAT I and II during the periods 1-30 June 1979 and 1-30 April 1982, respectively, over Europe and northern Africa. The method assumes basically that clouds perturb the ?clear sky? radiance fields. Thus, the satellite data of reflected solar radiation are used as indicators for the presence of clouds and of their transparency for radiation scattered upward from underneath. Radiative transfer calculations have been employed to determine clouds and atmospheric transmittance for solar radiation at different zenith angles. A comparison with simultaneous measurements of the European network of pyranometers yields rms differences of 0.25 kWh m?2 (June 1979) and 0.28 kWh m?2 (April 1982), respectively, for monthly averages of daily sums. This uncertainty corresponds to ?5?6% of the available insolation. Our results are available with a resolution of about 25?25 km2.
dc.publisherAmerican Meteorological Society
dc.titleIncident Solar Radiation over Europe Estimated from METEOSAT Data
dc.typeJournal Paper
dc.journal.volume23
dc.journal.issue1
dc.journal.titleJournal of Climate and Applied Meteorology
dc.identifier.doi10.1175/1520-0450(1984)023<0166:ISROEE>2.0.CO;2
dc.journal.fristpage166
dc.journal.lastpage170
dc.treeJournal of Climate and Applied Meteorology:;1984:;volume( 023 ):;issue: 001
dc.contenttypeFulltext


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