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Author Aubé, M.; Franchomme-Fossé, L.; Robert-Staehler, P.; Houle, V. url  doi
openurl 
  Title Light pollution modeling and detection in a heterogeneous environment: toward a night time aerosol optical depth retrieval method. Type Journal Article
  Year 2005 Publication Proceedings of SPIE 2005 -- Volume 5890, San Diego, California, USA. Abbreviated Journal  
  Volume 5890 Issue Pages  
  Keywords Skyglow; aerosol optical depth;  remote sensing; light pollution; artificial skyglow  
  Abstract Tracking the Aerosol Optical Depth (AOD) is of particular importance in monitoring aerosol contributions to global radiative forcing. Until now, the two standard techniques used for retrieving AOD were; (i) sun photometry, and (ii) satellite based approaches, such as based DDV (Dense Dark Vegetation) inversion algorithms. These methods are only available for use during daylight time since they are based on direct or indirect observation of sunlight. Few attempts have been made to measure AOD behaviour at night. One such method uses spectrally ­ calibrated stars as reference targets but the number of available stars is limited. This is especially true for urban sites where artificial lighting hides most  of these stars. In this research, we  attempt  to provide an alternate method, one  which exploits artificial sky glow or light pollution. This methodology links a 3D light pollution model with in situ light pollution measurements. The basic idea is to adjust an AOD value into the model in order to fit measured light pollution. This method requires an accurate model that includes spatial heterogeneity in lighting angular geometry, in lighting spectral dependence, in ground spectral reflectance and in topography. This model, named ILLUMINA, computes 1st and 2nd order molecular and aerosol scattering, as well as aerosol absorption. These model features represent major improvements to previous light pollution models. Therefore, new possibilities for light pollution studies will arise, many of which are of particular interest to the astronomical community. In this paper we will present a first sensitive study applied to the ILLUMINA model.  
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  Call Number LoNNe @ kagoburian @ Serial 554  
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Author Albers, S.; Duriscoe, D.M. url  openurl
  Title Modeling light pollution from population data and implications for National Park Service lands. Type Journal Article
  Year 2001 Publication George Wright Forum Abbreviated Journal  
  Volume 18 Issue Pages 56-68  
  Keywords Skyglow  
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  Notes Approved no  
  Call Number LoNNe @ kagoburian @ Serial 555  
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Author Cinzano, P.; Stagni, R. openurl 
  Title The colors of the sky glow. Type Journal Article
  Year 2000 Publication Mem Soc Astron Ita Abbreviated Journal  
  Volume 71 Issue Pages 231-234.  
  Keywords Skyglow  
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  Call Number LoNNe @ kagoburian @ Serial 557  
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Author Falchi, F.; Cinzano, P. openurl 
  Title Measuring and Modelling Light Pollution. Type Journal Article
  Year 2000 Publication Mem Soc Astron Ital Abbreviated Journal  
  Volume 71 Issue Pages 139  
  Keywords Skyglow  
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  Call Number LoNNe @ kagoburian @ Serial 558  
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Author Garstang, R.H. url  doi
openurl 
  Title Night-sky brightness at observatories and sites. Type Journal Article
  Year 1989 Publication Publ Astron Soc Pac Abbreviated Journal  
  Volume 101 Issue Pages 306-329  
  Keywords Skyglow  
  Abstract A model previously constructed for night-sky brightness calculations has been modified to allow for the curvature of the earth. The model has been applied to calculate the brightness at the following observatories: Mount Wilson, Lick, Mount Palomar, Kitt Peak, Sacramento Peak, Mauna Kea, McDonald, San Pedro Martir, Mount Hopkins, Mount Lemmon, Lowell (Mars Hill), Lowell (Anderson Mesa), Fick, Iowa, Van Vleck, David Dunlap, Anglo-Australian, Haute Provence, and Cerro Tololo. Calculations have also been carried out for the following prospective observatory sites: Junipero Serra, Mount Graham, Charleston Peak, Wheeler Peak, Miller Peak, San Benito Mountain, Lowell (Hutch Mountain), Lowell (Saddle Mountain), and South Baldy (New Mexico). The model is extended to calculate magnitudes in the B photometric band.  
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  Notes Approved no  
  Call Number LoNNe @ kagoburian @ Serial 559  
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