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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

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 present a method to map the artificial sky brightness across large territories in astronomical photometric bands with a resolution of approximately 1 km. This is useful to quantify the situation of night sky pollution, to recognize…

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

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

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

Artificial light at night is a pollutant that is rising fast, as demonstrated by Kyba et al. (1) work by analyzing ten of thousands observations by citizen scientists in the last 12 years. The study found that the dimmest stars are…

天体物理仪器与方法 · 物理学 2023-07-03 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

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

The population of artificial satellites and space debris orbiting the Earth imposes non-negligible constraints on both space operations and ground-based optical and radio astronomy. The ongoing deployment of several satellite…

天体物理仪器与方法 · 物理学 2021-04-02 Miroslav Kocifaj , Frantisek Kundracik , John C. Barentine , Salvador Bará

The total number and luminosity function of the population of dwarf galaxies of the Milky Way (MW) provide important constraints on the nature of the dark matter and on the astrophysics of galaxy formation at low masses. However, only a…

星系天体物理 · 物理学 2018-07-18 Oliver Newton , Marius Cautun , Adrian Jenkins , Carlos S. Frenk , John Helly

The visual perception of the natural night sky in many places of the world is strongly disturbed by anthropogenic light. Part of this artificial light is scattered in the atmosphere and propagates towards the observer, adding to the natural…

天体物理仪器与方法 · 物理学 2023-05-02 Salvador Bará , Carmen Bao-Varela

Light pollution is a worldwide problem that has a range of adverse effects on human health and natural ecosystems. Using data from the New World Atlas of Artificial Night Sky Brightness, VIIRS-recorded radiance and Gross Domestic Product…

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

Light pollution is recognized as a global issue that, like other forms of anthropogenic pollution, has significant impact on ecosystems and adverse effects on living organisms. Multiple evidence suggests that it has been increasing at an…

The Milky Way's (MW) satellite population is a powerful probe of warm dark matter (WDM) models as the abundance of small substructures is very sensitive to the properties of the WDM particle. However, only a partial census of the MW's…

星系天体物理 · 物理学 2019-11-01 Oliver Newton , Marius Cautun , Adrian Jenkins , Carlos S. Frenk , John C. Helly

Over the years, the Maltese Islands have seen a marked rise in the prevalence of artificial lighting at night. The most evident type of light pollution arising from this evolution in anthropogenic night-time lighting is artificial skyglow…

天体物理仪器与方法 · 物理学 2020-02-12 Joseph Caruana , Ryan Vella , Daniel Spiteri , Michael Nolle , Sara Fenech , Noel J. Aquilina

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

Artificial skyglow is constantly growing on a global scale, with potential ecological consequences ranging up to affecting biodiversity. To understand these consequences, worldwide mapping of skyglow for all weather conditions is urgently…

天体物理仪器与方法 · 物理学 2017-09-12 Andreas Jechow , Zoltán Kolláth , Salvador J. Ribas , Henk Spoelstra , Franz Hölker , Christopher C. M. Kyba

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
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