Identifying, Examining, and Planning Areas Protected from Light Pollution
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25 11.4 1.6 David Lubin Memorial Library
COPY FROM MICROFICHE RECORD OF DOCUMENTARY UNIT NO. : COPIE OE LA MICROriCHE DE L'UNITE DOCUMENTAIRE NO. : 3tn COPIA Did LA MICROFICHA DE LA UNITAO DOCUMENTAL NO. : — |'-8 • ' mmsÊBuJ x / ,25 11.4 1.6 FOOD AND AGRICULTURE ORGANIZATION OF THE UNITED NATIONS ORGANISATION DES NATIONS UNIES POUR L'ALIMENTATION ET L'AGRICULTURE ORGANIZACIÓN DE LAS NACIONES UNIDAS PARA LA AGRICULTURA Y LA ALIMENTACIÓN DAVID LUBIN MEMORIAL LIBRARY F AO • VU ¿ella Terme di'Caraealla - 00100 ROME. Italy We regret that„some of thé pages in the microfiche copy of this.report may not be up to the proper^'. ' legibility standards,even though the best possible-.: copy was used for preparing the master fiche. - r ¿6 frtkïL F AO- r AG:DP/GRE/77/023 ) l/\ j, )>>-/ Technical Report, Vol. I I v WATER RESOURCES DEVELOPMENT IN THE MOLAI AREA GREECE TECHNICAL REPORT Volume I: TEXT ftgfiß UNITED NATIONS DEVELOPMENT PROGRAMME FOOD AND AGRICULTURE ORGANIZATION OF THE UNITED NATIONS ROME, 1081 0 FAO - AGiDP/GRE/77/023 Technical Report WATER RESOURCES DEVELOPMENT IN THE MOLAI AREA GREECE TECHNICAL REPORT VOLUME I! TEXT Report prepared for the Government of Greece by the Food and Agriculture Organization of the United Nations acting as executing agency for the United Nations Development Programme UNITED NATIONS DEVELOPMENT PROGRAMME FOOD AND AGRICULTURE ORGANIZATION OF THE UNITED NATIONS Rome, 1981 Iii FAO. Water Resources Development in the Molai Area, Greece. Rome, 198T! 3 volb., 56 lip.iire«, ?¿ mnps. AG:DP/GRK/77/023, Technical Report. A BrTRACT The report describes the work carried out by the Government of Greece, with the assistance of I'KDP and FAO, to assess the availability of ground water Cor the irrigation of up to 6 000 ha tin the Molai plain, Lakónia. -
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 ........................................................................................ -
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. -
KARYES Lakonia
KARYES Lakonia The Caryatides Monument full of snow News Bulletin Number 20 Spring 2019 KARYATES ASSOCIATION: THE ANNUAL “PITA” DANCE THE BULLETIN’S SPECIAL FEATURES The 2019 Association’s Annual Dance was successfully organized. One more time many compartiots not only from Athens, but also from other CONTINUE cities and towns of Greece gathered together. On Sunday February 10th Karyates enjoyed a tasteful meal and danced at the “CAPETANIOS” hall. Following the positive response that our The Sparta mayor mr Evagellos first special publication of the history of Valliotis was also present and Education in Karyes had in our previous he addressed to the Karyates issue, this issue continues the series of congratulating the Association tributes to the history of our country. for its efforts. On the occasion of the Greek National After that, the president of the Independence Day on March 25th, we Association mr Michael publish a new tribute to the Repoulis welcome all the participation of Arachovitians/Karyates compatriots and present a brief in the struggle of the Greek Nation to report for the year 2018 and win its freedom from the Ottoman the new year’s action plan. slavery. The board members of the Karyates Association Mr. Valliotis, Sparta Mayor At the same time, with the help of Mr. The Vice President of the Association Ms Annita Gleka-Prekezes presented her new book “20th Century Stories, Traditions, Narratives from the Theodoros Mentis, we publish a second villages of Northern Lacedaemon” mentioning that all the revenues from its sells will contribute for the Association’s actions. special reference to the Karyes Dance Group. -
Southern Peloponnese Free
FREE SOUTHERN PELOPONNESE PDF Michael Cullen | 136 pages | 15 Mar 2015 | Sunflower Books | 9781856914512 | English | London, United Kingdom What to see in southern Peloponnese? - Peloponnese Forum - Tripadvisor It is connected to the central part of the country by the Isthmus of Corinth land bridge which separates the Gulf of Corinth from the Saronic Gulf. The peninsula is divided among three administrative regions : most belongs to the Peloponnese region, with smaller parts belonging to the West Greece and Attica regions. The Peloponnese is a peninsula that covers an area of some 21, It is connected to the mainland by the Isthmus of CorinthSouthern Peloponnese the Corinth Canal was constructed in However, it is also connected to the mainland by several bridges across the canal, including two submersible bridges at the north and the south Southern Peloponnese. Near the northern tip of the peninsula, there is another bridge, the Rio—Antirrio bridge completed Indeed, the Southern Peloponnese is rarely, if ever, referred to as an island. The peninsula has a mountainous interior and deeply indented coasts. The Peloponnese possesses four south-pointing peninsulas, the Messenianthe Manithe Cape Malea also known as Epidaurus Limeraand the Southern Peloponnese in the far northeast of the Peloponnese. The entire peninsula is earthquake prone and has been the site of many earthquakes in the past. Extensive lowlands are found only in the west, except for the Evrotas valley in the south and the Argolid in the northeast. Southern Peloponnese Peloponnese is home to numerous spectacular beaches, which are a major tourist draw. Two groups of islands lie off the Peloponnesian coast: the Argo-Saronic Islands to the east, and the Ionian to the west. -
Νέες Προσεγγίσεις Στην Αποκατάσταση Δασών Μαύρης Πεύκης» Σπάρτη, 15-16 Οκτωβρίου 2009
ΠΡΑΚΤΙΚΑ Διεθνές Συνέδριο «Νέες προσεγγίσεις στην αποκατάσταση δασών μαύρης πεύκης» Σπάρτη, 15-16 Οκτωβρίου 2009 PROCEEDINGS International Conference "New approaches to the restoration of black pine forests" Sparti, 15 - 16 October 2009 EPrO: LIFE07 NAT/GR/00286 NATURA 2 0 0 0 ΠΡΑΚΤΙΚΑ Διεθνές Συνέδριο «Νέες προσεγγίσεις στην αποκατάσταση δασών* "» Α μαύρηςΛ πευκης»Λ Σπάρτη, 15-16 Οκτωβρίου 2009 PROCEEDINGS International Conference "New approaches to the restoration of black pine forests" Sparti, 15 - 16 October 2009 Η παρούσα έκδοση έγινε στο πλαίσιο του έργου Life07 NAT/GR/000286 «Αποκατάσταση των δασών Pinus nigra στον Πάρνωνα (GR2520006) μέσω μίας δομημένης προσέγγισης» (www.parnonaslife.gr) που υλοποιείται από το Ελληνικό Κέντρο Βιοτόπων - Υγροτόπων (Δικαιούχος), την Περιφέρεια Πε- λοποννήσου, τον Φορέα Διαχείρισης Όρους Πάρνωνα και Υγροτόπου Μουστου και την Περιφέρεια Ανατολικής Μακεδονίας και Θράκης (Εταίροι). To έργο χρηματοδοτείται από τη ΓΔ Περιβάλλον της Ευρωπαϊκής Επιτροπής, τη Γενική Διευθυνση Ανάπτυξης και Προστασίας Δασών και Φυσικου Περι βάλλοντος, τον Δικαιούχο και τους Εταίρους. The present publication has been prepared in the framework of the Life07 NAT/GR/000286 «Restoration of Pinus nigra forests on Mount Parnonas (GR2520006) through a structured approach» (www.parnonaslife.gr) which is implemented by the Greek Biotope - Wetland Centre (Coordinating Beneficiary), the Region of Peloponnisos, the Management Body of mount Parnonas and Moustos wetland and the Region of Eastern Macedonia - Thrace (Associated Beneficiaries). -
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 ................................................................................................................................................