Next Article in Journal
Volcanic Ash, Insecurity for the People but Securing Fertile Soil for the Future
Next Article in Special Issue
Identifying, Examining, and Planning Areas Protected from Light Pollution. The Case Study of Planning the First National Dark Sky Park in Greece
Previous Article in Journal
Multi-Objective and Multi-Attribute Optimization for Sustainable Development Decision Aiding
Previous Article in Special Issue
Observing the Impact of WWF Earth Hour on Urban Light Pollution: A Case Study in Berlin 2018 Using Differential Photometry
Open AccessArticle

Monitoring Long-Term Trends in the Anthropogenic Night Sky Brightness

Departmento Física Aplicada, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Galicia
Physics, School of Health of the Polytechnic Institute of Porto, 4200-072 Porto, Portugal
CITEUC—Centre for Research on Earth and Space of the University of Coimbra, Observatório Astronómico da Universidade de Coimbra, 3030-004 Coimbra, Portugal
Departamento de Física de la Tierra y Astrofísica, Instituto de Física de Partículas y del Cosmos (IPARCOS), Universidad Complutense de Madrid, 28040 Madrid, Spain
Author to whom correspondence should be addressed.
Sustainability 2019, 11(11), 3070;
Received: 26 April 2019 / Revised: 27 May 2019 / Accepted: 28 May 2019 / Published: 31 May 2019
Monitoring long-term trends in the evolution of the anthropogenic night sky brightness is a demanding task due to the high dynamic range of the artificial and natural light emissions and the high variability of the atmospheric conditions that determine the amount of light scattered in the direction of the observer. In this paper, we analyze the use of a statistical indicator, the mFWHM, to assess the night sky brightness changes over periods of time larger than one year. The mFWHM is formally defined as the average value of the recorded magnitudes contained within the full width at half-maximum region of the histogram peak corresponding to the scattering of artificial light under clear skies in the conditions of a moonless astronomical night (sun below −18°, and moon below −5°). We apply this indicator to the measurements acquired by the 14 SQM detectors of the Galician Night Sky Brightness Monitoring Network during the period 2015–2018. Overall, the available data suggest that the zenithal readings in the Sky Quality Meter (SQM) device-specific photometric band tended to increase during this period of time at an average rate of +0.09 magSQM/arcsec2 per year. View Full-Text
Keywords: light pollution measurement; radiometry; photometry; environmental monitoring; sky brightness light pollution measurement; radiometry; photometry; environmental monitoring; sky brightness
Show Figures

Figure 1

MDPI and ACS Style

Bará, S.; Lima, R.C.; Zamorano, J. Monitoring Long-Term Trends in the Anthropogenic Night Sky Brightness. Sustainability 2019, 11, 3070.

Show more citation formats Show less citations formats
Note that from the first issue of 2016, MDPI journals use article numbers instead of page numbers. See further details here.

Article Access Map by Country/Region

Search more from Scilit
Back to TopTop