Night-sky radiometry can revolutionize the characterization of light-pollution sources globally

The city emission function (CEF), describing the angular emission from an entire city as a light source, is one of the key elements in night-sky radiance models. The CEF describes the rate at which skyglow depends on distance and is indispensable in any prediction of light-pollution propagation into...

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Detalles Bibliográficos
Autor: HECTOR ANTONIO SOLANO LAMPHAR
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:México
Institución:Centro de Investigación e Innovación en Tecnologías de la Información y Comunicación
Repositorio:Repositorio Institucional de INFOTEC
Idioma:inglés
OAI Identifier:oai:infotec.repositorioinstitucional.mx:1027/540
Acceso en línea:http://infotec.repositorioinstitucional.mx/jspui/handle/1027/540
Access Level:acceso abierto
Palabra clave:info:eu-repo/classification/Autoridades UNAM/Medidas ópticas
info:eu-repo/classification/Autoridades UNAM/Radiación -- Medición
info:eu-repo/classification/Autoridades UNAM/Contaminación
info:eu-repo/classification/Autoridades UNAM/Contaminación lumínica
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/21
info:eu-repo/classification/cti/2103
info:eu-repo/classification/cti/220911
Descripción
Sumario:The city emission function (CEF), describing the angular emission from an entire city as a light source, is one of the key elements in night-sky radiance models. The CEF describes the rate at which skyglow depends on distance and is indispensable in any prediction of light-pollution propagation into nocturnal environments. Nevertheless, the CEF remains virtually unexplored because appropriate retrieval tools have been unavailable until very recently. A CEF has now been obtained from ground-based night-sky observations and establishes an experiment successfully conducted in the field to retrieve the angular emission function for an urban area. The field campaign was conducted near the city of Los Mochis, Mexico, which is well isolated from other cities and thus dominates all light emissions in its vicinity. The experiment has proven that radiometry of a night sky can provide information on the light output pattern of a distant city and allows for systematic, full-area, and cost-efficient CEF monitoring worldwide. A database of CEFs could initiate a completely new phase in light-pollution research, with significant economy and advanced accuracy of night-sky brightness predictions. The experiment and its interpretation represent unique progress in the field and contribute to our fundamental understanding of the mechanism by which direct and reflected uplight interact while forming the CEF.