2014
DOI: 10.1093/mnras/stu1577
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Particulate matter as an amplifier for astronomical light pollution

Abstract: In this paper, we state that the main factor that influences seasonal changes in the brightness of the cloudless, moonless, light-polluted night sky is primarily particulate matter, emitted mainly from low-emission sources, especially in winter. This effect is particularly noticeable in Cracow and its surroundings, one of the places in Europe that is most polluted by particulate matter. Measurements taken over a period of one year have allowed us to show a linear relationship between the concentration of parti… Show more

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Cited by 20 publications
(7 citation statements)
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“…Daytime aerosol optical depth (AOD) measurements show a slight decrease in the last hours before the nights of measurement from 2017 to 2020 (see Appendix C). The absence of polluting aerosols will reduce skyglow as shown in a study in Cracow, Poland [24], but also means less extinction towards the satellite, which is exactly what we have observed.…”
Section: Discussionsupporting
confidence: 86%
“…Daytime aerosol optical depth (AOD) measurements show a slight decrease in the last hours before the nights of measurement from 2017 to 2020 (see Appendix C). The absence of polluting aerosols will reduce skyglow as shown in a study in Cracow, Poland [24], but also means less extinction towards the satellite, which is exactly what we have observed.…”
Section: Discussionsupporting
confidence: 86%
“…Until recently, understanding of typical levels and patterns of skyglow has been extremely poor. The invention of robust and easy to use light meters like the “Sky Quality Meter” (SQM; Unihedron), however, has resulted in a boom in skyglow measurement 29 30 31 32 33 34 35 36 37 38 39 40 . This has led to some understanding of patterns on a local scale, and emphasized the need for comparative studies across different regions.…”
mentioning
confidence: 99%
“…Given the fact that the calculation of atmospheric diffuse flux is a rather complicated problem that requires a detailed treatment of multiple scatterings (Kocifaj & Bará 2019) and knowledge of atmospheric composition such as aerosols, ozone and particulate matter (Joseph et al 1991;Ściężor & Kubala 2014;Ściężor & Czaplicka 2020). it is expected that the residuals of Δ mdl−obs show discrepancies.…”
Section: Models and Methodsmentioning
confidence: 99%