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We present the map of the artificial sky brightness in Europe in V band with a resolution of approximately 1 km. The aim is to understand the state of night sky pollution in Europe, to quantify the present situation and to allow future…

天体物理学 · 物理学 2007-05-23 P. Cinzano , F. Falchi , C. D. Elvidge , K. E. Baugh

We present a project to map the artificial sky brightness in Europe in the main astronomical photometrical bands with a resolution better than 3 km. The aim is to understand the state of night sky pollution in Europe, to quantify the…

天体物理学 · 物理学 2007-05-23 P. Cinzano , F. Falchi , C. D. Elvidge , K. E. Baugh

We apply the sky brightness modelling technique introduced and developed by Roy Garstang to high-resolution DMSP-OLS satellite measurements of upward artificial light flux and to GTOPO30 digital elevation data in order to predict the…

天体物理学 · 物理学 2009-11-10 Pierantonio Cinzano , Cristopher D. Elvidge

We obtained the map of the zenith brightness of the night sky in Italy. The artificial sky brightness in each site is computed by integration of the contributions by each unitary area of surface obtained by applying a propagation function…

天体物理学 · 物理学 2007-05-23 F. Falchi , P. Cinzano

Knowledge of the night sky radiance over a large territory may be valuable informationto identify sites appropriate to astronomical observations or for assessing the impacts ofartificial light at night on ecosystems. Measuring the sky…

天体物理仪器与方法 · 物理学 2021-04-28 Alexandre Simoneau , Martin Aubé , Jérôme Leblanc , Rémi Boucher , Johanne Roby , Florence Lacharité

Modeling the hemispherical night sky brightness of anthropogenic origin is a demanding computational challenge, due to the intensive calculations required to produce all-sky maps with fine angular resolution including high-order scattering…

天体物理仪器与方法 · 物理学 2022-03-30 Miroslav Kocifaj , Salvador Bará , Fabio Falchi

Ground-based optical astronomy necessarily involves sensing the light of astronomical objects along with the contributions of many natural sources ranging from the Earth's atmosphere to cosmological light. In addition, astronomers have long…

天体物理仪器与方法 · 物理学 2022-08-31 John C. Barentine

Measuring the brightness of the night sky has become an increasingly important topic in recent years, as artificial lights and their scattering by the Earths atmosphere continue spreading around the globe. Several instruments and techniques…

Methods to map artificial night sky brightness and stellar visibility across large territories or their distribution over the entire sky at any site are based on the computation of the propagation of light pollution with Garstang models, a…

天体物理仪器与方法 · 物理学 2016-09-05 Pierantonio Cinzano , Fabio Falchi

Artificial lights raise night sky luminance, creating the most visible effect of light pollution-artificial skyglow. Despite the increasing interest among scientists in fields such as ecology, astronomy, health care, and land-use planning,…

We extend the method introduced by Cinzano et al. (2000a) to map the artificial sky brightness in large territories from DMSP satellite data, in order to map the naked eye star visibility and telescopic limiting magnitudes. For these…

天体物理学 · 物理学 2009-10-31 P. Cinzano , F. Falchi , C. D. Elvidge

A crucial part of the qualification of international dark sky places (IDSPs) is the objective measurement of night time sky luminance or radiance. Modern digital cameras provide an alternative way to perform all sky imaging either by a…

天体物理仪器与方法 · 物理学 2017-05-29 Zoltán Kolláth , Anita Dömény

We describe a system for rapidly measuring the brightness of the night sky using a mosaic of CCD images obtained with a low-cost automated system. The portable system produces millions of independent photometric measurements covering the…

天体物理学 · 物理学 2009-11-13 D. M. Duriscoe , C. B. Luginbuhl , C. A. Moore

Several light pollution indicators are commonly used to monitor the effects of the transition from outdoor lighting systems based on traditional gas-discharge lamps to solid-state light sources. In this work we analyze a subset of these…

天体物理仪器与方法 · 物理学 2019-09-25 Salvador Bará , Iago Rigueiro , Raul C. Lima

Nighttime monitoring of the aerosol content of the lower atmosphere is a challenging task, because appropriate reference natural light sources are lacking. Here we show that the anthropogenic night sky brightness due to city lights can be…

天体物理仪器与方法 · 物理学 2020-11-18 Miroslav Kocifaj , Salvador Bará

The sustained increase of emissions of artificial light is causing a progressive brightening of the night sky in most of the world. This process represents a threat for the long-term sustainability of the scientific and educational activity…

天体物理仪器与方法 · 物理学 2020-12-29 Fabio Falchi , Salvador Bará

Contrary to some widespread intuitive belief, the night sky brightness perceived by the human eye or any other physical detector does not come (exclusively) from high in the sky. The detected brightness is built up from the scattered…

天体物理仪器与方法 · 物理学 2023-02-03 Salvador Bará , Carmen Bao-Varela , Miroslav Kocifaj

The knowledge of the contribution $b_d(d)$ to the artificial sky luminance in a given point of the sky of a site produced by the sources beyond a given distance $d$ from it is important to understand the behaviour of light pollution in…

天体物理学 · 物理学 2007-05-23 P. Cinzano

Modelling techniques for the propagation of light pollution in the atmosphere allow the computation of maps of artificial night sky brightness in any direction of the sky, involving a large number of details from satellite data. Cinzano et…

天体物理仪器与方法 · 物理学 2020-07-02 Pierantonio Cinzano , Fabio Falchi

Light pollution is a form of environmental degradation in which excessive artificial outdoor lighting, such as street lamps, neon signs, and illuminated signboards, affects the natural environment and the ecosystem. Poorly designed outdoor…

天体物理仪器与方法 · 物理学 2014-03-24 Chun Shing Jason Pun , Chu Wing So , Wai Yan Leung , Chung Fai Wong
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