Light Pollution: Assessment of Sky Glow on Two Dark Sky Regions of Portugal
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Environmental and Social Data Sheet
Luxembourg, 20 July 2018 Public Environmental and Social Data Sheet Overview Project Name: TAMEGA IBERDROLA HYDROPOWER AND STORAGE PORTUGAL Project Number: 2015-0651 Country: Portugal Project Description: The project concerns the construction of 3 new large dams and 3 hydropower plants with a total capacity of 1,158 MW in the Douro River Basin in northern Portugal. EIA required: yes Project included in Carbon Footprint Exercise1: yes Environmental and Social Assessment The Project is located on Tâmega River and Torno River, within the Douro river basin, in Northern Portugal, 90 km of Porto. The Project construction works shall be completed by June 2023. The Project comprises the following components: 1. Alto Tâmega HPP: 108m arch dam with a monthly reservoir (470ha, 131.7 hm3) and 160 MW, 87m head, 200 m3/s power plant; 2. Daivões HPP: 77m arch gravity dam with a weekly reservoir (340ha, 56.2hm3) and 118 MW, 65m head, 227 m3/s power plant; 3. Gouvães PSP: 32m gravity dam with a daily reservoir (176ha, 12.7hm3) and 880 MW, 657m head, 160 m3/s pumped -storage plant; 4. The associated facilities inter alia access roads, 20kV overhead lines. 5. A quarry located in Gouvães; 6. 400kV grid connection facilities including 400kV Gouvães susbstation and around 15km overhead lines connecting the three sites to the point of delivery, Ribeira de Pena substation. In addition, in order to evacuate the power of the Project from Ribeira de Pena substation to the national grid, the Portuguese transmission system operator Redes Energética Nacionais (REN) will upgrade the national grid in Grande Porto area and build new 132 km 400kV overhead lines Feira – Ribeira de Pena – Vieira do Minho. -
GLOBE at Night: Using Sky Quality Meters to Measure Sky Brightness
GLOBE at Night: using Sky Quality Meters to measure sky brightness This document includes: • How to observe with the SQM o The SQM, finding latitude and longitude, when to observe, taking and reporting measurements, what do the numbers mean, comparing results • Demonstrating light pollution o Background in light pollution and lighting, materials needed for the shielding demo, doing the shielding demo • Capstone activities (and resources) • Appendix: An excel file for multiple measurements CREDITS This document on citizen-scientists using Sky Quality Meters to monitor light pollution levels in their community was a collaborative effort between Connie Walker at the National Optical Astronomy Observatory, Chuck Bueter of nightwise.org, Anna Hurst of ASP’s Astronomy from the Ground Up program, Vivian White and Marni Berendsen of ASP’s Night Sky Network and Kim Patten of the International Dark-Sky Association. Observations using the Sky Quality Meter (SQM) The Sky Quality Meters (SQMs) add a new twist to the GLOBE at Night program. They expand the citizen science experience by making it more scientific and more precise. The SQMs allow citizen-scientists to map a city at different locations to identify dark sky oases and even measure changes over time beyond the GLOBE at Night campaign. This document outlines how to make and report SQM observations. Important parts of the SQM ! Push start button here. ! Light enters here. ! Read out numbers here. The SQM Model The SQM-L Model Using the SQM There are two models of Sky Quality Meters. Information on the newer model, the SQM- L, can be found along with the instruction sheet at http://unihedron.com/projects/sqm-l/. -
International Dark Sky Parks Guidelines
INTERNATIONAL DARK-SKY ASSOCIATION 3223 N First Ave - Tucson Arizona 85719 USA - +1 520-293-3198 - www.darksky.org TO PRESERVE AND PROTECT THE NIGHTTIME ENVIRONMENT AND OUR HERIT- AGE OF DARK SKIES THROUGH ENVIRONMENTALLY RESPONSIBLE OUTDOOR LIGHTING International Dark Sky Park Program Guidelines June 2018 IDA International Dark Sky Park Designation Guidelines TABLE OF CONTENTS DEFINITION OF AN IDA DARK SKY PARK .................................................................. 3 GOALS OF DARK SKY PARK CREATION ................................................................... 3 DESIGNATION BENEFITS ............................................................................................ 3 ELIGIBILITY ................................................................................................................... 4 MINIMUM REQUIREMENTS FOR ALL PARKS ............................................................ 5 LIGHTING MANAGEMENT PLAN ................................................................................. 8 LIGHTING INVENTORY ............................................................................................... 10 PROVISIONAL STATUS .............................................................................................. 12 IDSP APPLICATION PROCESS .................................................................................. 13 NOMINATION ........................................................................................................... 13 STEPS FOR APPLICANT ........................................................................................ -
National Report Portugal
NATIONAL REPORT PORTUGAL | August 2016 TECHNICAL TEAM Coordinator Cristina Cavaco Coordination Team DGT António Graça Oliveira, Cristina Gusmão, Margarida Castelo Branco, Margarida Nicolau, Maria da Luz França, Maria do Rosário Gaspar, Marta Afonso, Marta Magalhães, Nuno Esteves, Ricardo Gaspar Network of Focal Points Habitat III Albano Carneiro (AMP), Alexandra Castro (ISS), Alexandra Sena (CCDR-ALG), Alexandre N. Capucha (DGTF), Álvaro Silva (IPMA), Ana C. Fernandes (APA), Ana Galelo (IMT), Ana Santos (AMP), Ana Veneza (CCDR-C), António M. Perdição (DGADR), Avelino Oliveira (AMP), Carla Benera (IHRU), Carla Velado (CCDR-C), Carlos Pina (CCDR-LVT), Conceição Bandarrinha (AML), Cristina Faro (IEFP), Cristina Guimarães (CCDR-N), Cristina Magalhães (ANMP), Demétrio Alves (AML), Dina Costa Santos (ACSS), Dulce Gonçalves Dias (DGAL), Elsa Costa (ANPC), Elsa Soares (INE), Fernanda do Carmo (ICNF), Francisco Chagas Reis (ICNF), Francisco Vala (INE), Gabriel Luís (LNEG), Gonçalo Santos (ACSS), Graça Igreja (IHRU), Guilherme Lewis (DGADR), Hélder Cristóvão (IMT), Hernâni H. Jorge (RAA), Isabel Elias (CCIG), Isabel Rodrigues (IHRU), João José Rodrigues (RAM), João Lobo (REN-SA), João Pedro Gato (DGAL), José Correia (AML), José Freire (CCDR-N), José Macedo (CCDR-A), Linda Pereira (CCDR-LVT), Luís Costa (AML), Margarida Bento (CCDR-C), Maria João Lopes (ANMP), Maria João Pessoa (CCDR-N), Miguel Arriaga (DGS), Mónica Calçada (AdP), Nuno F. Gomes (ISS), Nuno Portal (EDP), Pedro Ribeiro (DGS), Ricardo Fernandes (ANSR), Rita Ribeiro (APA), Rui Gouveia -
Night Sky Monitoring Program for the Southeast Utah Group, 2003
NIGHT SKY United States Department of MONITORING Interior National Park Service PROGRAM Southeast Utah Group SOUTHEAST UTAH GROUP Resource Management Division Arches National Park Canyonlands National Park Moab Hovenweep National Monument Utah 84532 Natural Bridges National Monument General Technical Report SEUG-001-2003 2003 January 2004 Charles Schelz / SEUG Biologist Angie Richman / SEUG Physical Science Technician EXECUTIVE SUMMARY NIGHT SKY MONITORING PROGRAM Southeast Utah Group Arches and Canyonlands National Parks Hovenweep and Natural Bridges National Monuments Project Funded by the National Park Service and Canyonlands Natural History Association This report lays the foundation for a Night Sky Monitoring Program in all the park units of the Southeast Utah Group (SEUG). Long-term monitoring of night sky light levels at the units of the SEUG of the National Park Service (NPS) was initiated in 2001 and has evolved steadily through 2003. The Resource Management Division of the Southeast Utah Group (SEUG) performs all night sky monitoring and is based at NPS headquarters in Moab, Utah. All protocols are established in conjunction with the NPS National Night Sky Monitoring Team. This SEUG Night Sky Monitoring Program report contains a detailed description of the methodology and results of night sky monitoring at the four park units of the SEUG. This report also proposes a three pronged resource protection approach to night sky light pollution issues in the SEUG and the surrounding region. Phase 1 is the establishment of methodologies and permanent night sky monitoring locations in each unit of the SEUG. Phase 2 will be a Light Pollution Management Plan for the park units of the SEUG. -
Measuring Night Sky Brightness: Methods and Challenges
Measuring night sky brightness: methods and challenges Andreas H¨anel1, Thomas Posch2, Salvador J. Ribas3,4, Martin Aub´e5, Dan Duriscoe6, Andreas Jechow7,13, Zolt´anKollath8, Dorien E. Lolkema9, Chadwick Moore6, Norbert Schmidt10, Henk Spoelstra11, G¨unther Wuchterl12, and Christopher C. M. Kyba13,7 1Planetarium Osnabr¨uck,Klaus-Strick-Weg 10, D-49082 Osnabr¨uck,Germany 2Universit¨atWien, Institut f¨urAstrophysik, T¨urkenschanzstraße 17, 1180 Wien, Austria tel: +43 1 4277 53800, e-mail: [email protected] (corresponding author) 3Parc Astron`omicMontsec, Comarcal de la Noguera, Pg. Angel Guimer`a28-30, 25600 Balaguer, Lleida, Spain 4Institut de Ci`encies del Cosmos (ICCUB), Universitat de Barcelona, C.Mart´ıi Franqu´es 1, 08028 Barcelona, Spain 5D´epartement de physique, C´egep de Sherbrooke, Sherbrooke, Qu´ebec, J1E 4K1, Canada 6Formerly with US National Park Service, Natural Sounds & Night Skies Division, 1201 Oakridge Dr, Suite 100, Fort Collins, CO 80525, USA 7Leibniz-Institute of Freshwater Ecology and Inland Fisheries, 12587 Berlin, Germany 8E¨otv¨osLor´andUniversity, Savaria Department of Physics, K´arolyi G´asp´ar t´er4, 9700 Szombathely, Hungary 9National Institute for Public Health and the Environment, 3720 Bilthoven, The Netherlands 10DDQ Apps, Webservices, Project Management, Maastricht, The Netherlands 11LightPollutionMonitoring.Net, Urb. Ve¨ınatVerneda 101 (Bustia 49), 17244 Cass`ade la Selva, Girona, Spain 12Kuffner-Sternwarte,Johann-Staud-Straße 10, A-1160 Wien, Austria 13Deutsches GeoForschungsZentrum Potsdam, Telegrafenberg, 14473 Potsdam, Germany Abstract Measuring the brightness of the night sky has become an increasingly impor- tant topic in recent years, as artificial lights and their scattering by the Earth’s atmosphere continue spreading around the globe. -
AM205: Syllabus
AM205: Data fitting for imaging Comet NEOWISE In late July 2020, Comet NEOWISE was visible from Earth. From a dark sky location, the comet was easily visible to the naked eye, and there were many superb photos that were taken showing the intricate structure of its tail. Chris has been fascinated by astronomy since an early age. His homewown of Keswick in the United Kingdom has very little light pollution, and he was able to appreciate won- ders of the night sky. However, from his current home near Central Square in Cambridge, Massachusetts there are high levels of light pollution and the sky usually appears a dim grey with all but the brightest stars washed out. On the Bortle scale that is used to measure light pollution [1], Cambridge ranks at roughly 7–8. Chris has a Fuji XT-4 digital camera, which has excellent image quality, but typical pictures of the night sky have a bright grey background. Figure1 shows a typical raw camera image, and it is difficult to make out any detail beyond the brightest stars. Further problems like aircraft lights and brightly lit clouds are also visible. As students of AM205, we can ask ourselves if it is possible to do better. The light pollution adds a smooth, but spatially varying, background to the image. Can we use our data fitting skills to subtract this out and reveal more detail? Figure 1: An example of the difficulty of night sky imaging from an urban area. This image with a 6.5 s exposure was taken near the MIT sports fields on August 11, 2020. -
Gower AONB - Dark Sky Quality Survey
Dark Sky Wales Allan Trow 28 December 2017 Gower AONB - Dark Sky Quality Survey Dark Sky Wales Training Services were commissioned in December 2017 by Swansea Council to undertake a baseline study of dark sky quality within the Gower AONB. The study was undertaken during December 2018 on clear and moonless nights. The following report highlights the findings from the study and includes recommendations for progressing Dark Sky activities in the area. !1 Introduction Light pollution through inappropriate or excessive use of artificial light makes it increasingly difficult to observe the night skies; indeed, over 90% of the UK population now lives under highly light-polluted skies. Dark skies contribute significantly to human health and wellbeing with increasing evidence showing that sleep is often disturbed by a lack of proper darkness at night with adverse impacts for health. Light pollution also impacts adversely on around 60% of wildlife, which is most active at night. In addition, sympathetic and energy-efficient lighting in communities can satisfy community needs at lower cost whilst importantly reducing carbon emissions. Dark skies are increasingly important for tourism through landscapes that offer unblemished views of the night sky. To support this aim, the AONB commissioned Dark Sky Wales in December 2017 to: • Work closely with AONB staff to identify 40 locations evenly spread across the area of interest. • Undertake study during moonless nights to ensure accurate readings are achieved without any natural influences. • Monitor weather conditions and attempt to undertake study on clear nights (some cloud cover can be worked around) • Use a minimum of two IDA1 standard SQM2 readers at each location • Take three readings from each machine to derive an average for the site. -
Studying Light Pollution in and Around Tucson, AZ
Utah State University DigitalCommons@USU Physics Capstone Project Physics Student Research Summer 2013 Studying Light Pollution in and Around Tucson, AZ Rachel K. Nydegger Utah State University Follow this and additional works at: https://digitalcommons.usu.edu/phys_capstoneproject Part of the Physics Commons Recommended Citation Nydegger, Rachel K., "Studying Light Pollution in and Around Tucson, AZ" (2013). Physics Capstone Project. Paper 3. https://digitalcommons.usu.edu/phys_capstoneproject/3 This Report is brought to you for free and open access by the Physics Student Research at DigitalCommons@USU. It has been accepted for inclusion in Physics Capstone Project by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. Studying Light Pollution in and around Tucson, AZ KPNO REU Summer Report 2013 Rachel K. Nydegger Utah State University, Kitt Peak National Observatory, National Optical Astronomy Observatory Advisor: Constance E. Walker National Optical Astronomy Observatory ABSTRACT Eight housed data logging Sky Quality Meters (SQMs) are being used to gather light pollution data in southern Arizona: one at the National Optical Astronomy Observatory (NOAO) in Tucson, four located at cardinal points at the outskirts of the city, and three situated at observatories on surrounding mountain tops. To examine specifically the effect of artificial lights, the data are reduced to exclude three natural contributors to lighting the night sky, namely, the sun, the moon, and the Milky Way. Faulty data (i.e., when certain parameters were met) were also excluded. Data were subsequently analyzed by a recently developed night sky brightness model (Duriscoe (2013)). During the monsoon season in southern Arizona, the SQMs were removed from the field to be tested for sensitivity to a range of wavelengths and temperatures. -
A Guide to Smartphone Astrophotography National Aeronautics and Space Administration
National Aeronautics and Space Administration A Guide to Smartphone Astrophotography National Aeronautics and Space Administration A Guide to Smartphone Astrophotography A Guide to Smartphone Astrophotography Dr. Sten Odenwald NASA Space Science Education Consortium Goddard Space Flight Center Greenbelt, Maryland Cover designs and editing by Abbey Interrante Cover illustrations Front: Aurora (Elizabeth Macdonald), moon (Spencer Collins), star trails (Donald Noor), Orion nebula (Christian Harris), solar eclipse (Christopher Jones), Milky Way (Shun-Chia Yang), satellite streaks (Stanislav Kaniansky),sunspot (Michael Seeboerger-Weichselbaum),sun dogs (Billy Heather). Back: Milky Way (Gabriel Clark) Two front cover designs are provided with this book. To conserve toner, begin document printing with the second cover. This product is supported by NASA under cooperative agreement number NNH15ZDA004C. [1] Table of Contents Introduction.................................................................................................................................................... 5 How to use this book ..................................................................................................................................... 9 1.0 Light Pollution ....................................................................................................................................... 12 2.0 Cameras ................................................................................................................................................ -
Mobilidade E Transportes No Grande Porto
Revista da Faculdade de Letras — Geografia I série, vol. XV/XVI, Porto, 1999-2000, pp. 7 - 17 Mobilidade e transportes no Grande Porto Maria da Luz Costa1 1. Considerações introdutórias A finalidade de um sistema de transporte de passageiros é a movimentação de pessoas, não a movimentação de veículos. A movimentação de veículos, a sua paragem e estacionamento, é um meio para atingir este objectivo, não um objectivo em si. Em termos económicos, de gestão do espaço urbano, de segurança, de energia e ambiental, é sempre desejável atingir essa finalidade com um número mínimo de veículos. As características dos diferentes segmentos do mercado de deslocações, conjugadas com as vocações específicas de cada um dos modos de transporte, deverão determinar o equilíbrio correcto na repartição e na complementaridade dos modos de transporte de passageiros. Este equilíbrio é obviamente influenciado e induzido pelas condições e quantidade de oferta atribuídas a cada modo de transporte e pelos sistemas globais dos transportes públicos e individuais: muitas decisões de repartição modal são tomadas não em função de uma única deslocação, mas sim em função de um conjunto de deslocações quotidianas do agregado familiar. Para os utilizadores de transportes, o custo, o tempo e o conforto da deslocação têm uma influência decisiva na escolha da modalidade de transporte. Todavia, os utilizadores de automóveis originam uma série de custos em que eles próprios não incorrem e que, por isso, não consideram quando decidem como vão deslocar-se. Estes custos incluem impactes ambientais, como, por exemplo, a poluição sonora e do ar, e aspectos associados a acidentes, congestionamentos, utilização do espaço, entre outros. -
Snowglow—The Amplification of Skyglow by Snow and Clouds Can
Journal of Imaging Article Snowglow—The Amplification of Skyglow by Snow and Clouds Can Exceed Full Moon Illuminance in Suburban Areas Andreas Jechow 1,2,* and Franz Hölker 1,3 1 Ecohydrology, Leibniz-Institute of Freshwater Ecology and Inland Fisheries, 12587 Berlin, Germany 2 Remote Sensing, GFZ German Research Centre for Geosciences, 14473 Potsdam, Germany 3 Institute of Biology, Freie Universität Berlin, 14195 Berlin, Germany * Correspondence: [email protected] Received: 27 June 2019; Accepted: 29 July 2019; Published: 1 August 2019 Abstract: Artificial skyglow, the fraction of artificial light at night that is emitted upwards from Earth and subsequently scattered back within the atmosphere, depends on atmospheric conditions but also on the ground albedo. One effect that has not gained much attention so far is the amplification of skyglow by snow, particularly in combination with clouds. Snow, however, has a very high albedo and can become important when the direct upward emission is reduced when using shielded luminaires. In this work, first results of skyglow amplification by fresh snow and clouds measured with all-sky photometry in a suburban area are presented. Amplification factors for the zenith luminance of 188 for snow and clouds in combination and 33 for snow alone were found at this site. The maximum zenith luminance of nearly 250 mcd/m2 measured with snow and clouds is a factor of 1000 higher than the commonly used clear sky reference of 0.25 mcd/m2. Compared with our darkest zenith luminance of 0.07 mcd/m2 measured for overcast conditions in a very remote area, this leads to an overall amplification factor of ca.