Index of /~jhollan/light/drafts/graphics

[ICO]NameLast modifiedSizeDescription

[PARENTDIR]Parent Directory  -  
[DIR]italian/2011-08-11 13:57 -  
[   ]scatt_en.pdf2003-04-04 22:50 5.6K 
[   ]scatt_en_wb.pdf2007-10-30 11:31 6.6K 
[   ]scatt_cz.lan.eps2005-02-25 12:40 9.4K 
[   ]scatt_en.lan.eps2005-02-25 12:40 9.4K 
[   ]scatt_cz.eps2005-02-25 12:40 9.4K 
[   ]scatt_en.eps2011-08-10 19:17 9.5K 
[   ]scatt_cz.pdf2003-04-04 22:50 18K 
[IMG]scatt_en_wb.png2013-04-16 20:01 61K 
[IMG]scatt_en.88.png2003-04-04 22:50 72K 
[IMG]scatt_cz.png2004-02-07 17:03 84K 
[   ]scatt_all.zip2004-02-07 17:07 177K 

This is a draft graphics explaining where the artificial skyglow comes from. The numbers are valid for ``CIE sky No. 5'' type of scattering (indicatrix function, to be accurate), usual for a clear, but not extremely clear sky, and for ``zenith extinction'' of 0.3 mag.

The scheme is written as a Postscript code and is easy to adapt to other languages then Czech and English as well. It could be used to illustrate the topic dealt with in e.g. my lp_quant3 draft, see http://amper.ped.muni.cz/light/drafts/ directory.