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Lunar Skylight Polarization Signal Polluted by Urban Lighting. Christopher Kyba 1,2 , Thomas Ruhtz 1 , Jürgen Fischer 1 , Franz Hölker 2 1 Freie Universität Berlin 2 Leibniz-Institute of Freshwater Ecology and Inland Fisheries 11th Dark Sky Symposium, Osnabruck Oct 6, 2011. - PowerPoint PPT Presentation
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Lunar Skylight Polarization Signal Polluted by Urban Lighting
Christopher Kyba1,2, Thomas Ruhtz1, Jürgen Fischer1, Franz Hölker2
1Freie Universität Berlin2Leibniz-Institute of Freshwater Ecology and
Inland Fisheries
11th Dark Sky Symposium, Osnabruck Oct 6, 2011
Verlust der Nacht(Loss of the Night)
• Collaboration of 9 Universities / Institutes
• 14 Integrated Subprojects
• Many aspects of light pollution considered, from measurement to ecology to sociology
http://userpage.fu-berlin.de/~kyba/Light pollution conferences
Twitter: @skyglowberlinYoutube: skyglowberlin
Outline
• Polarization of light
• Nocturnal insect navigation
• Experiment setup
• Results and interpretation
• Ecological consequences
How does light become polarized?
• Polarization is a characteristic of light
• Most sources produce unpolarized light
• Horizontally polarized light generated by reflections
• Linearly polarized light generated through Rayleigh scattering
How does light become polarized?
Nocturnal Navigation
Dacke et al. 2003
• Dung beetles navigate using the polarized sky light of the moon
• Signal strength seven orders of magnitude smaller than in daytime
Properties of sky polarization
• Degree of linear pol. is strongest at twilight• Twilight band of maximum polarization
runs approximately North/South• Moonlight polarization pattern almost
identical to sunlight p.p. (Gál et al. 2001)• Polarization pattern is visible in partly
cloudy skies (Pomozi et al. 2001)
=> Polarization is a more robust directional signal than the sun, moon, or stars
Experimental Setup
• Berlin is at 52oN• North Star is 38o from zenith• Moon’s max deviation from
ecliptic is 18o-28o
• Moon is always 62o to 118o from North Star (66o to 114o in 2010)
• North Star is always near peak of Rayleigh polarization
• Geometry is independent of position on Earth, and changes a few degrees/day
Measurement Locations
50 km
• Compare lunar skylight polarization at urban and rural location
• Brandenburg is very dark compared to Berlin
N
Measurement equipmentSigma 24mm f1.8
tripod
SC4022LPFCFW-8
Blue Red
Note: Measure each LPF position (at least) 4x for each filter
Skyglow pollutes lunar polarization signal!
Degree of linear polarization
Urban moonrise: 3.9 ± 0.2%Urban with moon: 11.3 ± 0.3%Rural moon: 29.2 ± 0.8%Urban daytime: 56.6 ± 1.0%Laboratory (LCD): 98.1 ± 1.2%
Skyglow pollutes lunar polarization signal!
Degree of linear polarizationUrban no moon: 8.6 ± 0.3%Urban moonrise: 3.9 ± 0.2%Urban with moon: 11.3 ± 0.3%Rural moon: 29.2 ± 0.8%Urban daytime: 56.6 ± 1.0%Laboratory (LCD): 98.1 ± 1.2%
?!?!?
Should skyglow be polarized?
• Most sources of light pollution are unpolarized
• Horizontally polarized light scattered upwards
• Rayleigh scattering can direct light downwards
• Sources of light pollution are spatially distributed
• Light pollution is generally uncollimated
Naively, no
What do simulations say?
• Skyglow simulations describe propagation of light from sources to observer
• Most do not take polarization into account
• The simulation that does (Kerola 2006) predicts that skyglow is almost unpolarized (~2%)
Aubé 2007
But skyglow can be polarized!
• Moonless, clear sky observing conditions
• Similar values observed several months apart
• Results for one particular direction in one city
Degree of linear polarization370-510 nm: 10.1 ± 0.5%490-580 nm: 9.4 ± 0.7%590-690 nm: 8.5 ± 1.4%370-700 nm: 8.6 ± 0.3%
How can this be?
Ecological consequences
• Nocturnal insect navigation– dung beetles– crickets?– moths?– bees?
• Bird attraction to searchlights?
Dacke et al. 2003
Conclusions
• Skyglow pollutes the natural polarization signal of the moon
• Extremely likely to affect navigational abilities of some nocturnal insects
• Skyglow itself can be weakly polarized
• Skyglow polarization could be used for remote sensing of aerosols at night
Acknowledgements
Photo CreditsTable: Briho (Wikimedia Commons)
Sky: Christopher KybaDragonfly: Andreas Trepte (WC)Waggle dance: Jüppsche (WC)
Skyglow: Jeremy StanleyGlacier National Park: Ray Stinson
New York City: CharlieBrown7034 (WC)Light pollution map: WEW/FU Berlin
Light pollution model: Martin Aubé (2007)
FundingBMBF 033L038A
MILIEU (FU Berlin)
Thank you!
Polarization of daytime skylight
Rayleigh scattering
(Pomozi et al. 2001)
Measuring Stokes Vector
When this is done for every pixel, you have imaging polarimetry
SearchlightsVisual brightness
(blue band)Degree of
linear polarization
Animal use of polarized light:Migration
• Birds use polarization cues to re-calibrate their magnetic compass daily
• Average of sunset and sunrise is true North, and independent of latitude and time of year
• Experiments hold birds in altered magnetic field during twilight
• Birds look for this cue preferably at the horizon
Mulheim et al. 2006Cochran et al. 2004
Animal use of polarized light:Material detection
• Water detection is most well known use
• Leads to “polarized light pollution” from artificial surface reflections (Horváth et al. 2009)
• Acquatic animals also use it in hunting