Panoramas à 360° des dômes de pollution lumineuse

4th Dark-Sky European Symposium, Paris, September 24-25, 2004

Content

nAims

nMeans

nA typical result

nSensibility to the location : correlation to the Cinzano/Falchi/Elvidge/Baugh Atlas of the artificial night sky brightness

nSensibility to the location : moving a few kilometers away

nSensibility to the night hour : 3 hours apart

nSensibility to the time of the year

nSensibility to the meteorological conditions

nConclusion and perspectives


	Here is the content.
	After exposing the way the night sky pictures are acquired, I will show you what kind of information may be derived from them. Especially if there is some correlation between these field recordings, and the Cinzano Atlas of the artificial night sky brightness.
	We’ll see also in any improvement in the sky transparency may be expected with the night hour, the season in the year, or the meteorological conditions.