Solar and Terrestrial Radiation 1975
DOI: 10.1016/b978-0-12-192950-3.50011-5
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Polarization of Light in the Atmosphere

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Cited by 106 publications
(227 citation statements)
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References 35 publications
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“…At the latitude of Panama near the equator, astronomical twilight starts about 1 h before local sunrise and ends about 1 h after local sunset. During the entire twilight period the polarisation pattern varies little in angular distribution, degree of polarisation, or spectral content, reaching an 80% degree of polarisation at wavelengths of 600 nm (Coulson 1988;Cronin et al 2006). Thus, with the high polarisation sensitivity present in the DRA of the nocturnal bee M. genalis, the polarisation pattern during this twilight period represents a simple and reliable orientation cue.…”
Section: Polarised Light As a Nocturnal Navigation Cuementioning
confidence: 92%
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“…At the latitude of Panama near the equator, astronomical twilight starts about 1 h before local sunrise and ends about 1 h after local sunset. During the entire twilight period the polarisation pattern varies little in angular distribution, degree of polarisation, or spectral content, reaching an 80% degree of polarisation at wavelengths of 600 nm (Coulson 1988;Cronin et al 2006). Thus, with the high polarisation sensitivity present in the DRA of the nocturnal bee M. genalis, the polarisation pattern during this twilight period represents a simple and reliable orientation cue.…”
Section: Polarised Light As a Nocturnal Navigation Cuementioning
confidence: 92%
“…The spectrum of celestial polarised skylight at night, both from the sun and the moon, peaks at middle to long wavelengths (Coulson 1988;Gal et al 2001;Barta and Horvath 2004;Cronin etal. 2006).…”
Section: Polarised Light As a Nocturnal Navigation Cuementioning
confidence: 99%
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“…An angle of view of 180 ø was ensured by a fisheye lens (NikonNikkor, F-2.8, focal length: 8 ram) including a built-in rotating disc mounted with three neutral density linear polarization (type HNP'B) filters with three different polarization axes (0 ø, 45 ø, and 90 ø measured from the radius of the disc), and the detector was a photoemul- 26ø30'E *The solar azimuth angle c; was the same as the lunar azimuth angle in Table 1. As the polarization of scattered sunlight [Coulson, 1988], also the polarization of scattered moonlight depends slightly on the wavelength [Gehrels, 1974]. This sinall wavelength dependency of the polarization patterns of the moonlit clear night sky was washed out by using black and white photographic film as detector: In order to minimize the time of exposure, the polarization characteristics of the moonlit sky must have been recorded by a highly sensitive photographic film.…”
Section: Measurement Of the Celestial Polarizationmentioning
confidence: 99%
“…julien.serres@univ-amu.fr constituents induce the partially linear polarization of the skylight [3]. As shown in figure 1, the direction of the linear polarization of skylight at the zenith point is always perpendicular to the solar meridian.…”
Section: Introductionmentioning
confidence: 92%