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LPLAB: Laboratory of Photometry and Radiometry of Light Pollution www.lplab.it Cinzano 2003, Mem. Soc. Astron. It. Suppl., 3, 312-315
Main steps OLS-DMSP Reduction of radiance data Data analysis Geographical and spatial distribution of upward light emission Atmosphere Earth-based measurements Modelling of light pollution propagation Map computation Validation of results Night sky brightness Stellar visibility Changes with time Correlation with the geographical distribution of population
Page 1 and 2: Recent progresses on a Second World
Page 3: Funding for this project and relate
Page 7 and 8: New Computational techniques Cinzan
Page 9 and 10: EGM account for: multiple scatterin
Page 11 and 12: The software package LPTRAN (Light
Page 13 and 14: New Computational techniques New ou
Page 15 and 16: New indicators of light pollution:
Page 17 and 18: Illuminance/irradiance at soil from
Page 19 and 20: No biunivocal relation between the
Page 21 and 22: We want improve the validation with
Page 23 and 24: Response Sky Quality Meter Characte
Page 25 and 26: Night Sky Brightness (mag/arcsec^2)
Page 27 and 28: 3) solution of primary issues of ph
Page 29 and 30: New Computational techniques New ou
Page 31 and 32: We want improve our knowledge of th
Page 33 and 34: study of growth of light pollution
Page 35: Convegno Rotary, Sant'Agata Feltria
Page 38 and 39: Lights in Cekia Pizen Dresda Usti P
Page 40 and 41: Magnitude loss in Cekia Cinzano/IST
Page 42 and 43: Roadpollution v. beta 1.5 a free so

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