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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…

We present a study of the night sky brightness around the extended metropolitan area of Madrid using Sky Quality Meter (SQM) photometers. The map is the first to cover the spatial distribution of the sky brightness in the center of the…

In the last decade numerous Sky Quality Meters (SQMs) were installed throughout the globe, aiming to assess the temporal change of the night sky brightness (NSB), and thus the change in light pollution. However, it has become clear that SQM…

天体物理仪器与方法 · 物理学 2021-02-10 Johannes Puschnig , Magnus Näslund , Axel Schwope , Stefan Wallner

Light pollution is an increasing environmental concern, impacting both ecological systems and human health. This report presents an analysis of light pollution data from the washetdonker.nl SQM network from 2020 until 2023, with a focus on…

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

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

The Sky Brightness Monitor (SBM) is an important instrument to measure the brightness level for the sky condition, which is a critical parameter for judging a site for solar coronal observations. In this paper we present an automatic method…

太阳与恒星天体物理 · 物理学 2015-06-22 M. Y. Zhao , Y. Liu , A. Elmhamdi , A. S. Kordi , H. A. Al-trabulsy , X. F. Zhang , T. F. Song , S. Q. Liu , Y. D. Shen , Z. J. Tian , Y. H. Miao

Long-term monitoring of the evolution of the artificial night sky brightness is a key tool for developing science-informed public policies and assessing the efficacy of light pollution mitigation measures. Detecting the underlying…

天体物理仪器与方法 · 物理学 2020-12-02 Salvador Bará , Enric Marco , Salvador J. Ribas , Manuel Garcia Gil , Alejandro Sánchez de Miguel , Jaime Zamorano

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

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

Continuously monitored quantum systems are emerging as promising platforms for quantum metrology, where a central challenge is to identify measurement strategies that optimally extract information about unknown parameters encoded in the…

量子物理 · 物理学 2026-02-11 Alejandro Vivas-Viaña , Carlos Sánchez Muñoz

We present long-term (4-10 years) trends of light pollution observed at 26 locations, covering rural, intermediate and urban sites, including the three major European metropolitan areas of Stockholm, Berlin and Vienna. Our analysis is based…

天体物理仪器与方法 · 物理学 2022-10-26 Johannes Puschnig , Stefan Wallner , Axel Schwope , Magnus Näslund

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

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

This paper presents multi-filter measurements of the night sky brightness at the South African Astronomical Observatory (SAAO) in Sutherland in the presence of a bright moon. The observations cover a wide range of sky directions, lunar…

天体物理仪器与方法 · 物理学 2022-05-25 Hartmut Winkler

Results of the first comprehensive light pollution survey in Hong Kong are presented. The night-sky brightness was measured and monitored around the city using a portable light sensing device called the Sky Quality Meter over a 15-month…

天体物理仪器与方法 · 物理学 2012-03-05 Chun Shing Jason Pun , Chu Wing So

The use of Synthetic Aperture Radar (SAR) has greatly advanced our capacity for comprehensive Earth monitoring, providing detailed insights into terrestrial surface use and cover regardless of weather conditions, and at any time of day or…

信号处理 · 电气工程与系统科学 2024-02-05 Francesco Mauro , Alessandro Sebastianelli , Maria Pia Del Rosso , Paolo Gamba , Silvia Liberata Ullo

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

Quantum optics potentially offers an information channel from the Universe beyond the established ones of imaging and spectroscopy. All existing cameras and all spectrometers measure aspects of the first-order spatial and/or temporal…

天体物理学 · 物理学 2015-06-24 Dainis Dravins

The number of satellites on low orbit has dramatically increased over the past years, raising concerns among the astronomical community about their impact on observations. Spectroscopic observations represent a large fraction of…

天体物理仪器与方法 · 物理学 2024-01-19 Olivier R. Hainaut Sabine Moehler
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