NoeFlandre/osm-polygon-wikidata-only huggingface dataset:
Desert Sunrise High School

Desert Sunrise High School is a comprehensive public high school in Maricopa, Arizona, in the United States. The school is in the Maricopa Unified School District, and is located on Murphy Rd and Farrell Rd in Maricopa. Its school mascot is Gary the Golden Hawk, and its colors are blue and gold. Desert Sunrise opened in July 2022 with grades 9 and 10 for the 2022-23 school year. Grade 11 was added for the 2023-24 school year, followed by grade 12 for the 2024-25 school year. History In 2018, about $26 million was approved by the School Facilities Board to construct a second high school in the Maricopa Unified School District. The school district noticed a growing student population and the need for additional classroom space. It was designed by the Orcutt Winslow architectural firm and was built by Chasse Building Team. Ground was broken on May 7, 2021. The school will be built in three phases. The first phase consists of classroom space that can be scaled up as the student population grows. It also includes a gymnasium and cafeteria. A third building houses the administrative offices. A soft opening was held on May 24, 2022. On the same day, ground was broken for phase 2, which includes sporting facilities, a building for a library, counseling offices, and a performance stage. Phase 2 opened at the beginning of the 2023-2024 school year. Future plans include additional classrooms, an arts complex, and a career and technical education building. RED Awards In March 2024, Desert Sunrise received top honors at the 2024 Real Estate Development Awards in the K-12 category. AgriScience Greenhouse In April 2024, it was announced that a greenhouse would be constructed for the school's AgriScience program, and it would be used for various student projects. Acid Fume Exposure and Evacuation On October 24, 2024, students at Desert Sunrise High School were evacuated to the school parking lot sometime around 10:24 a.m. due to exposure to salicylic acid fumes in a science classroom. Students returned to classes around 11:36, after a response to the situation by the Maricopa police and fire departments. Parents were promptly notified about the situation and were asked to monitor their children for "any signs of breathing difficulty over the next 24 hours." References External links Official website
HonorHealth Scottsdale Osborn Medical Center

HonorHealth Scottsdale Osborn Medical Center is a private, non-profit acute-care teaching hospital, a part of the HonorHealth network in Scottsdale, Arizona. History The hospital was founded in 1962. In 2021, the hospital opened the 250,000-square-foot Bob Bové Neuroscience Center. Facilities The hospital is an American College of Surgeons-verified Level I trauma center, an Arizona Department of Health Services-certified cardiac arrest center, and a DNV-certified primary stroke center. The campus is also home to the 15,500 square foot HonorHealth Military Partnership Program training center. References External links HonorHealth Scottsdale Osborn Medical Center
Very Long Baseline Array

Very Long Baseline Array (VLBA) je systém deseti radioteleskopů dálkově kontrolovaných Array Operations Center ve městě Socorro, Nové Mexiko (USA), které spadá pod National Radio Astronomy Observatory. Systém pracuje na principu interferometrie a jedná se o největší systém svého druhu. Budování tohoto systému započalo v únoru 1986 a dokončen byl v květnu 1993. Observace, která využila všech deseti komponentů proběhla 23. května 1993. Celková cena stavby činila 85 milionů USD. Každý komponent sestává z jedné antény s průměrem paraboly 25m a přilehlé kontrolní budovy, ve které se nachází řídící počítač, páskové záznamníky a další vybavení, které souvisí se záznamem signálů přijatých anténou. Hmotnost každé antény činí 240 tun a jsou téměř stejně vysoké jako desetipodlažní dům. Nejdelší základní linie systému činí 8611 km. Lokace jednotlivých komponentů: Mauna Kea, Havaj Owens Valley, Kalifornie Kitt Peak, Arizona Pie Town, Nové Mexiko Los Alamos, Nové Mexiko Fort Davis, Texas Brewster, Washington North Liberty, Iowa Hancock, New Hampshire Saint Croix, Americké Panenské ostrovy Odkazy Reference V tomto článku byl použit překlad textu z článku Very Long Baseline Array na anglické Wikipedii. Související články Radioastronomie Radioteleskop Very Large Array Very Small Array Externí odkazy Obrázky, zvuky či videa k tématu Very Long Baseline Array na Wikimedia Commons Oficiální web projektu
Very Long Baseline Array

Das Very Long Baseline Array (VLBA) ist ein Radiointerferometer, mit dem nach den Verfahren der VLBI Radiobeobachtungen astronomischer Objekte mit höchster Winkelauflösung gewonnen werden können. Die zehn Antennen des VLBA mit je 25 m Durchmesser und 240 Tonnen Gewicht sind über zehn Standorte in den USA verteilt: Mauna-Kea-Observatorium, Hawaii Owens Valley Radio Observatory, Kalifornien Brewster, Washington North Liberty, Iowa Hancock, New Hampshire Kitt-Peak-Nationalobservatorium, Arizona Pie Town, New Mexico Fort Davis, Texas Los Alamos, New Mexico Saint Croix (Amerikanische Jungferninseln) Die größte Entfernung zwischen diesen Standorten ist 8611 km. Die Antennen verfügen über Empfänger für zehn Frequenzbereiche zwischen 1,2 und 96 GHz. Durch die langen Basislinien zwischen den Standorten erreicht das VLBA, je nach Frequenz, eine Winkelauflösung von teilweise weniger als einer tausendstel Bogensekunde. Mit dem Bau des VLBA wurde 1986 begonnen. Das VLBA wurde 1993 eingeweiht und wird vom National Radio Astronomy Observatory der USA betrieben. Die Zentrale befindet sich in Socorro, am Standort des Very Large Array. Weblinks Offizielle Webseite (englisch)
Very Long Baseline Array

Le Very Long Baseline Array (traduisible par le réseau à très longue ligne de base) est un réseau américain de radiotélescopes astronomiques fonctionnant dans le domaine 330 MHz à 86 GHz, pour faire de l'interférométrie à très longue base. Le VLBA comprend 10 antennes de 25 mètres chacune, et couvrant le territoire américain depuis Sainte-Croix dans les Îles Vierges, situées dans les Antilles et le Mauna Kea sur l'île d'Hawaï dans l'océan Pacifique. Le centre des opérations se trouve à Socorro au Nouveau-Mexique (États-Unis). Liste des antennes Lien externe (en) Site officiel du VLBA. Portail de l’astronomie Portail des États-Unis
Very Long Baseline Array

Il Very Long Baseline Array (VLBA) è ad oggi il più grande radiotelescopio interferometrico esistente al mondo. Venne inaugurato nel 1994 dal National Radio Astronomy Observatory e costò circa 85 milioni di dollari. Caratteristiche tecniche È costituito da 10 antenne radio del diametro di 25 m sparse in tutto il territorio degli Stati Uniti d'America, dalle Isole Hawaii alle Isole Vergini Americane. Collettivamente, essi funzionano come un singolo telescopio di oltre 8000 km di diametro. Gli astronomi registrano i segnali (sincronizzati con un orologio atomico) e più tardi li mescolano con l'aiuto del calcolatore utilizzando la tecnica di interferometria chiamata interferometria a lunghissima base (VLBI). Se si aggiungono anche i segnali provenienti da un satellite giapponese per radioastronomia, il diametro effettivo del sistema si espande di conseguenza fino a oltre 20000 km. Per le lunghezze d'onda radio, il sistema produce immagini persino più dettagliate del telescopio spaziale Hubble. Di fatto, è così sensibile che anche la deriva dei continenti diventa apprezzabile in alcune osservazioni. Posizionamento delle antenne radio Le antenne radio sono dislocate nei seguenti stati: Mauna Kea - Isole Hawaii (presso l'Osservatorio di Mauna Kea) Brewster - Washington Valle di Owens - California Kitt Peak - Arizona Pie Town - Nuovo Messico Los Alamos - Nuovo Messico Fort Davis - Texas North Liberty - Iowa Hancock - New Hampshire Saint Croix - Isole Vergini Americane Risultati e ricerca scientifica Utilizzando i dati raccolti nel biennio 2014-2015, un gruppo di ricerca a guida italiana ha misurato direttamente la distanza di una regione di formazione stellare, G007.47+00.05 dalla parte opposta della Via Lattea rispetto al Sole, a circa 66.000 al. Tale rilevazione, effettuata mediante misurazione della parallasse stellare, ha raddoppiato la precedente distanza rilevata con tale metodo. A luglio 2018 un gruppo di ricerca del Carnegie Institution for Science di Pasadena, California, ha scoperto il quasar PSO J352.4034-15.3373, al momento dell'osservazione era l'oggetto cosmico più brillante alle frequenze radio, ad una distanza di 13 miliardi di anni luce dalla terra. Galleria d'immagini Note Voci correlate Radioastronomia Altri progetti Wikimedia Commons contiene immagini o altri file su Very Long Baseline Array Collegamenti esterni (EN) Sito ufficiale, su public.nrao.edu. (EN) Very Long Baseline Array, su Enciclopedia Britannica, Encyclopædia Britannica, Inc.
Very Long Baseline Array

Het Very Long Baseline Array (VLBA) is een interferometer bestaande uit tien radiotelescopen die bestuurd worden vanuit Socorro (New Mexico). Het VLBA maakt deel uit van het National Radio Astronomy Observatory (NRAO). De tien telescopen werken samen door middel van Very-long-baseline interferometry. De bouw van het VLBA begon in februari 1986 en werd voltooid in mei 1993. De eerste astronomische waarnemingen met alle tien telescopen zijn gedaan op 29 mei 1993. De kosten van de bouw van het VLBA waren 85 miljoen dollar. Elke ontvanger van het VLBA bestaat uit een radiotelescoop met een diameter van 25 meter (gewicht 218 ton), en een gebouwtje waarin zich de elektronica en computers voor besturing en data opslag bevinden. De metingen krijgen een 'tijdstempel' met behulp van een atoomklok en worden opgestuurd naar Socorro waar ze in het Pete V. Domenici Science Operations Center verder verwerkt worden. Hierbij wordt rekening gehouden met kleine afwijkingen in de rotatie van de aarde en met bewegingen van de aardkorst. Metingen met het VLBA kunnen gedaan worden in acht banden met golflengtes tussen 3 mm en 90 cm (frequentie 96 - 0,3 GHz), afhankelijk van het object waarin men geïnteresseerd is. Telescopen De tien VLBA telescopen bevinden zich in: Mauna Kea-observatorium, Hawaï Owens Valley Radio Observatory, bij Big Pine, Californië Brewster, Washington North Liberty, Iowa Hancock, New Hampshire Kitt Peak National Observatory, Arizona Pie Town, New Mexico Fort Davis, Texas Los Alamos, New Mexico Saint Croix, Amerikaanse Maagdeneilanden De langste basislijn (afstand tussen twee telescopen) van het VLBA is 8611 km (Mauna Kea - Saint Croix). High-Sensitivity Array Voor hogere resolutie en/of gevoeligheid kunnen ook VLBI metingen gedaan worden in samenwerking met andere telescopen: de Arecibo telescoop in Puerto Rico, de Green Bank Telescope in West Virginia, het Very Large Array (VLA) in New Mexico, en de Radiotelescoop Effelsberg in Duitsland. Dit wordt het High-Sensitivity Array genoemd. Externe link website VLBA
Very Long Baseline Array

Very Long Baseline Array (VLBA) – system 10 radioteleskopów z centrum zdalnego sterowania (ang. Array Operations Center) położonym w Socorro w stanie Nowy Meksyk w USA, które podlega pod National Radio Astronomy Observatory. Radioteleskopy współpracują jako największy wyspecjalizowany, pełnoetatowy instrument astronomiczny, wykorzystujący technikę interferometrii wielkobazowej. Jego budowa rozpoczęła się w lutym 1986, a została ukończona w maju 1993. Pierwsza obserwacja wykorzystująca wszystkie 10 jednostek miała miejsce 29 maja 1993. Całkowity koszt budowy wyniósł 85 milionów USD (ok. 160 mln USD w 2021). Każda stacja VLBA składa się z anteny satelitarnej o średnicy 25 metrów (82 stóp) i sąsiadującego z nią budynku sterowni, w którym znajduje się komputer stacji, magnetofony i inne urządzenia związane ze zbieraniem sygnałów radiowych, odbieranych przez antenę. Każda z anten waży 218 ton, a jej wysokość, gdy jest skierowana pionowo, jest porównywalna do wysokości 10-piętrowego budynku. Najdłuższa linia bazowa (odległość między stacjami) w systemie ma długość 8611 km, a najkrótsza 52 km. Radioteleskopy VLBA znajdują się w (w nawiasach kwadratowych zapisano skróty nazw): [MK] Mauna Kea, Hawaje () [BR] Brewster, Waszyngton () [OV] Owens Valley, Kalifornia () [KP] Kitt Peak, Arizona () [PT] Pie Town, Nowy Meksyk () [LA] Los Alamos, Nowy Meksyk () [FD] Fort Davis, Teksas () [NL] North Liberty, Iowa () [HN] Hancock, New Hampshire () [SC] Saint Croix, Wyspy Dziewicze Stanów Zjednoczonych () Dodatkowe 3 radioteleskopy i jeden system radioteleskopów są dołączane do VLBA przez okres do 100 godzin w przeciągu 4 miesięcy. W tej konfiguracji system nazywany jest High-Sensitivity Array. Radioteleskopy te to (w nawiasach kwadratowych zapisano skróty nazw): [Y27] Very Large Array, Nowy Meksyk () [GB] Radioteleskop Green Bank, Wirginia Zachodnia () [AR] Obserwatorium Arecibo, Portoryko () [EB] radioteleskop Effelsberg, Niemcy () Odległości i rozdzielczości kątowe Odległości pomiędzy radioteleskopami (km): Maksymalna rozdzielczość kątowa: Uwagi Przypisy Linki zewnętrzne Oficjalna strona VLBA. [dostęp 2009-11-14]. (ang.).
Very Long Baseline Array

O Very Long Baseline Array (VLBA) é um sistema de dez radiotelescópios que são operados remotamente a partir de seu centro de operações que está localizado em Socorro, Novo México, como parte do National Radio Astronomy Observatory (NRAO). Estas dez antenas de rádio trabalham juntas como uma matriz que forma o sistema mais longo do mundo que usa uma base de interferometria muito longa. A linha de base mais longa disponível neste interferômetro é de cerca de 8.611 quilômetros. A construção do VLBA começou em fevereiro de 1986 e foi concluída em maio de 1993. A primeira observação astronômica usando todas as dez antenas foi realizada em 29 de maio de 1993. O custo total de construção do VLBA foi cerca de 85 milhões dólares. Cada receptor do VLBA consiste em uma antena parabólica de 25 metros de diâmetro, juntamente com o seu edifício de controle adjacente. Este contém eletrônicos e máquinas para apoiar o receptor, incluindo a eletrônica de baixo ruído, computadores digitais, unidades de armazenamento de dados e máquinas para apontar a antena. Cada uma das antenas é quase tão alto quanto um prédio de dez andares quando a antena é apontada diretamente para cima, e cada antena pesa cerca de 218 toneladas. Localização das antenas Mauna Kea - Havaí (no Observatório de Mauna Kea) Brewster - Washington Owens Valley - Califórnia Kitt Peak - Arizona Pie Town - Novo México Los Alamos - Novo México Fort Davis - Texas North Liberty - Iowa Hancock - Nova Hampshire Saint Croix - Ilhas Virgens dos Estados Unidos Referências Ligações externas Official site
Very Long Baseline Array

Very Long Baseline Array (VLBA) — Антенная решётка со сверхдлинными базами — радиоинтерферометр, принадлежащий Национальной радиоастрономической обсерватории (NRAO) США. VLBA состоит из десяти радиотелескопов, контролируемых удалённо из центра управления, расположенного в Сокорро, Нью-Мексико (США). Массив антенн работает совместно, как самый большой в мире, посвящённый исключительно интерферометрическим наблюдениям. Сооружение VLBA началось в феврале 1986, и закончилось в мае 1993. Первое наблюдение с использованием всех десяти антенн было проведено 29 мая 1993. Полная стоимость проекта — 85 млн $. VLBA может использоваться для наблюдения и картографирования различных компактных радиоисточников с яркостной температурой выше ~106 K. Максимальная база, расстояние между отдельными радиотелескопами, сети VLBA составляет 8600 км. Радиотелескопы могут вести приём в десяти частотных диапазонах от 300 МГц до 86 ГГц. Каждый радиотелескоп VLBA оборудован антенной диаметром 25 метров (главное зеркало), весом 218 тонн и имеет высоту примерно с десятиэтажное здание. Отношение фокальной длины главного зеркала к его диаметру составляет 0,354. Контррефлектор Кассегрена диаметром 3,5 метра, имеющий асимметричную форму, используется для всех рабочих частот выше 1 ГГц. Первичный фокус главного зеркала применяется для приёма низких частот. Рядом с каждым радиотелескопом располагается здание контроля, в котором находится центральный управляющий компьютер радиотелескопа, записывающее устройство и другое оборудование, связанное с обработкой радиосигнала, принятого антенной. Сигналы от каждой антенны записываются в хранилище данных ёмкостью около одного терабайта на жёстких дисках, информация отмечена временными метками с использованием атомных часов. По мере того, как диски заполняются данными, их отправляют в Центр научных операций им. Пита Доменичи NRAO в Сокорро. Там проводится обработка сигналов на мощном наборе цифровых компьютеров, которые и выполняют интерферометрию. Эти компьютеры также вносят поправки на вращение Земли, небольшие сдвиги земной коры с течением времени и другие небольшие погрешности измерения. Радиотелескопы VLBA располагаются в следующих местах: Мауна-Кеа, Гавайи () Brewster, Вашингтон () Owens Valley, Калифорния () Национальная обсерватория Китт-Пик, Аризона () Пай-Таун, Нью-Мексико () Лос-Аламос, Нью-Мексико () Форт-Дейвис, Техас () North Liberty, Айова () Хэнкок, Нью-Гэмпшир () Санта-Крус (Виргинские острова) () См. также КВАЗАР — Российская РСДБ сеть Института прикладной астрономии РАН EVN — Европейская РСДБ сеть Список радиотелескопов Примечания Ссылки Официальный сайт КВАЗАР Официальный сайт VLBA Официальный сайт NRAO
Fry Pioneer Cemetery

Fry Pioneer Cemetery is the original cemetery in Fry, Arizona, which was the name of Sierra Vista prior to its renaming and incorporation in 1956. It is a half-acre site, and includes more than 200 known graves, most of which are unmarked. It has sparse vegetation and is surrounded by a chain-link fence. The cemetery is a mile east of Fort Huachuca, an active military installation, completely enclosed by urban development. It is located between Sixth and Seventh Streets in Fry, Arizona, which is an unincorporated community wholly within the bounds of the city of Sierra Vista. It is accessible from both Fry Boulevard and the State Highway 90 bypass. There is sparse vegetation, and no planned walkways or landscaping, having developed organically over the years. The entire cemetery is surrounded by a chain link fence, installed in the 1960s. There is an entrance on the west side. Inside the cemetery is a three-foot brick wall which encloses the family plot of Oliver Fry and his family. The family plot has thirteen graves, all of which have headstones, although one is broken and without an inscription. Outside the family plot, the vast majority of the graves are unmarked. Outside the historic cemetery there are other unmarked graves on the south and east side, some of which have been identified as the resting place of Yaqui Indians. Also outside the historic cemetery, on the east side of Seventh Street, under a commercial parking lot, lie more burial sites. The cemetery was established in 1919 when Oliver Fry buried his wife, Elizabeth. The cemetery was in general use between 1919 and 1958, but now is only open to burials of descendants of the Fry family. The latest interment was a great-granddaughter of Oliver and Elizabeth in 2005. References External links Media related to Fry Pioneer Cemetery at Wikimedia Commons
Skyline Regional Park

Skyline Regional Park is an 8700-acre mountain preserve located in west-central Maricopa County, Arizona. The park is at the southern edge of the White Tank Mountains, within the arid Sonora Desert. The park is on a 25-year lease from BLM to the city of Buckeye, after which it reverts to the city. Activities It opened in 2016 with seven miles of trails, which have expanded to over 20 miles with a of mix of hiking, biking and equestrian trails. The most popular trail is the four mile Turnbuckle Loop Trail. The Crest Mountain summit vista offers unobstructed views of the Sierra Estrella Mountains to the northeast, Gila Bend Mountains in the southwest and the Big Horn Mountains Wilderness and the Hassayampa Plain in the northwest. The Javelina summit offers unobstructed views of downtown Phoenix, the Sierra Estrallas and the extensive desert plains. The Skyline Crest trail contains the highest peak, at 3152 feet, with a key col of 2760 ft. Other amenities include ramadas and shaded picnic and dry camping areas. With clear desert nights and remoteness from urban lights, the park is known for its dark skies. Stargazing activities are regularly scheduled; the park hosts "Star Party" events where visitors can learn about the night sky from local astronomers. In 2018 the park added 0.6 miles of accessible trails that can be used by strollers and wheelchairs. Bicycles and horses are not allowed on these trails. These trails have educational interpretive panels about native plants and animals. Guided group hikes are scheduled monthly. Flora and fauna Also see: Flora of the Sonoran Desert Also see: Fauna of the Sonoran Desert The landscape is desert and mountain. Desert mule deer, javelina, desert fox, raptors and Sonoran Desert tortoise are found in the park. Vegetation includes ironwood, palo verde and mesquite trees; many types of cacti are also found. Geology Text adapted from Wikipedia article White Tank Mountains: "The mountains were formed through tectonic activities as part of a detachment fault ... about 30 million years ago. Fairly young in geologic terms, it has not been subject to the forces of erosion for long and retains an extremely rugged topography composed of rocky fault ridges and deep canyons. During seasonal heavy rainfall, accumulated water tends to rush rapidly through the steep canyons, over time scouring out a number of depressions or 'tanks' in the white granite near the base of the mountains." This text is used under Creative Commons Attribution-ShareAlike 3.0 Unported License. References
Apache Generating Station

The Apache Power Plant is a 626-megawatt coal power plant and natural gas powered plant near Willcox, Arizona, United States, about 80 miles east of Tucson, Arizona. The plant is jointly owned by Arizona Electric Power Cooperative (AEPCO). The plant began operations in 1964. In 2024, owner AEPCO announced that by 2027 they planned to stop using coal and only use natural gas to power the plant. See also List of power stations in Arizona References External links APS [1] Data on generation and fuel consumption from the Energy Information Administration Electricity Data Browser
Desert Hills

Desert Hills és una concentració de població designada pel cens dels Estats Units a l'estat d'Arizona. Segons el cens del 2000 tenia 2.183 habitants. Demografia Segons el cens del 2000, Desert Hills tenia 2.183 habitants, 997 habitatges, i 677 famílies La densitat de població era de 179 habitants/km². Dels 997 habitatges en un 17,8% hi vivien nens de menys de 18 anys, en un 55,7% hi vivien parelles casades, en un 7,5% dones solteres, i en un 32% no eren unitats familiars. En el 25,2% dels habitatges hi vivien persones soles el 12,8% de les quals corresponia a persones de 65 anys o més que vivien soles. El nombre mitjà de persones vivint en cada habitatge era de 2,19 i el nombre mitjà de persones que vivien en cada família era de 2,54. Per edats la població es repartia de la següent manera: un 16,6% tenia menys de 18 anys, un 5% entre 18 i 24, un 19,9% entre 25 i 44, un 31,1% de 45 a 60 i un 27,4% 65 anys o més. L'edat mediana era de 52 anys. Per cada 100 dones de 18 o més anys hi havia 99,5 homes. La renda mediana per habitatge era de 26.678 $ i la renda mediana per família de 32.685 $. Els homes tenien una renda mediana de 21.690 $ mentre que les dones 20.433 $. La renda per capita de la població era de 14.322 $. Aproximadament el 10,5% de les famílies i el 14,1% de la població estaven per davall del llindar de pobresa. Poblacions properes El següent diagrama mostra les poblacions més properes. Referències
Desert Hills

Desert Hills ist ein Census-designated place im Mohave County im US-Bundesstaat Arizona. Das U.S. Census Bureau hat bei der Volkszählung 2020 eine Einwohnerzahl von 2.764 ermittelt. Desert Hills hat eine Fläche von 12,2 km² und eine Bevölkerungsdichte von 227 Einwohnern je km². Der Ort liegt an der Arizona State Route 95. Einzelnachweise