2023
DOI: 10.1016/j.jqsrt.2023.108592
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Natural variation of the colour and spectrum of the night sky observed at a potential european reference site for dark skies

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Cited by 4 publications
(5 citation statements)
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“…The presence of the Galactic plane in that direction complicates the interpretation (as the Galactic starlight represents one of the most significant contributors to the natural NSB; Duriscoe 2013; Masana et al 2021) but this evidence could be a hint that even at higher elevation (i.e., for ZA 60°) ALAN may contribute up to ∼0.15 mag arcsec −2 to the NSB of the western horizon at FJNP. When observing under very dark conditions like the ones encountered at this site, the only technique able to confirm this kind of insight seems to be spectroscopy (Kolláth & Jechow 2023).…”
Section: Fray Jorge National Park (Fjnp)mentioning
confidence: 95%
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“…The presence of the Galactic plane in that direction complicates the interpretation (as the Galactic starlight represents one of the most significant contributors to the natural NSB; Duriscoe 2013; Masana et al 2021) but this evidence could be a hint that even at higher elevation (i.e., for ZA 60°) ALAN may contribute up to ∼0.15 mag arcsec −2 to the NSB of the western horizon at FJNP. When observing under very dark conditions like the ones encountered at this site, the only technique able to confirm this kind of insight seems to be spectroscopy (Kolláth & Jechow 2023).…”
Section: Fray Jorge National Park (Fjnp)mentioning
confidence: 95%
“…31 However, our SQC data do not allow us to firmly weight the relative contributions of artificial and natural sources: a diffuse light, already perceivable in the RGB frame and clearly visible in the NSB map, runs in fact across the entire horizon and suggests that during that observing night there was a fairly high airglow activity. Airglow is known to contribute significantly to the intrinsic variability of the natural sky (Kolláth & Jechow 2023; Duriscoe 2016), its composite and complex multiperiodicity being sensitive to both atmospheric and space weather factors (Grauer & Grauer 2021). As was the case for FJNP, under near-pristine conditions like those at LCO it becomes challenging to separate the artificial (observednatural) from the observed (natural + artificial) sky radiance in specific directions without any spatially resolved spectral information.…”
Section: Las Campanas Observatory (Lco)mentioning
confidence: 99%
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“…Sunlight has a continuous broadband spectrum comprising nearly all wavelengths spanning from UV radiation to the visible range and IR radiation, and the spectrum of moonlight is similar, although usually slightly shifted towards longer (red) wavelengths ( figure 2 a ). The exact spectra of sunlight and moonlight vary to some extent, depending for example on altitude [ 25 ], and airglow also affects the spectrum of the natural night sky [ 26 ].
Figure 2 Empirical or modelled data on light spectra in relation to surface waters (A. Jechow 2023, unpublished data).
…”
Section: Light Properties and Pollutionmentioning
confidence: 99%
“…The quantification and characterization of the quality of the night sky can be carried out through several methodologies [43]. The study developed by Ges et al [44] proposes night sky quality indices based on spectral measurements, and the study developed by Kolláth et al [45] does so through radiance measurements. However, they all allow for generating concepts and precise tools for evaluating light pollution.…”
Section: Introductionmentioning
confidence: 99%