Difference between revisions of "Old Main Page 2009 with first results"
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− | [[ | + | [[File:L14_Berlin_Feb_Mae_2009.png|thumb|First Berlin-measurements Feb to early March 2009. Horizontal line: value for full moon in zenith]] |
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brightening (light pollution). Previously know as [[Luxmeter]] | brightening (light pollution). Previously know as [[Luxmeter]] | ||
− | [[ | + | [[File:L12_TLS_26Sep_bis_7Nov2008.png|thumb|40 days of measurements at Tautenburg; non-stop from 26th Sept. to 7th Nov. 2008.]] |
'''Note:''' To get access to all pages mail ''Verein@Kuffner-Sternwarte.at'' for a login. | '''Note:''' To get access to all pages mail ''Verein@Kuffner-Sternwarte.at'' for a login. |
Revision as of 14:50, 28 April 2016
File:== How many stars can we still see? - The starlight wiki ==
How many stars can we still see?: Simple naked eye sightings of the Little Dipper or Orion serve to determine the quality of the world's night skies.
Lightmeter: A network of newly-developed, low-cost lightmeters starts the global continuous monitoring of artificial night sky brightening (light pollution). Previously know as Luxmeter
Note: To get access to all pages mail Verein@Kuffner-Sternwarte.at for a login.
- What is Light Pollution? by Jan Hollan
- La Palma Deklaration und Nacht/Sternschutzgebiete (Starlight-Reserve)
- Beobachten
- Nachthimmelsschutz - LichtVerschmutzung
- Plan 2009
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21:07, 2. Apr. 2009 GuentherWuchterl