NoeFlandre/osm-polygon-wikidata-only huggingface dataset:
Izumo Taishakyo Mission of Hawaii

The Izumo Taishakyo Mission is a Shinto shrine located in downtown Honolulu, Hawaii. It is one of the few active Shinto shrines in the United States. The wooden A-frame structure was inspired by Shimane Prefecture's classical Japanese shrine Izumo-taisha. It was designed by architect Hego Fuchino and built by master carpenter Ichisaburo Takata. The primary kami of this shrine is Ōkuninushi and Hawaii Ubusuna-no-Kami. Also enshrined are Okinawa Shrine, Naminoue Shrine, Futenma Shrine, Inari Shrine, and Ebisu Shrine, and Waianae Ujigami. The shrine is the site of the annual New Year's Day hatsumōde as well as other events throughout the year. A replica of the Hiroshima Peace Bell is on view. The annual Hiroshima Commemoration and Peace Service is held at Hawaii Izumo Taisha to commemorate the atomic bombing of Hiroshima. History Hawaii Izumo Taisha was founded in 1906 when Rev. Katsuyoshi Miyao opened a temporary worship site on Aala Street near Aala Park on 26 September 1906. A temporary shrine building was completed on 25 August 1907. A permanent shrine building was completed in 1922. By 1941, there were branches of Izumo Taishakyo operating in Hilo, Wailuku, Waipahu, Pearl City, Honouliuli, Ewa Lower Camp, Aiea, and Kakaako. The shrine was closed on 7 December 1941 at the outset of World War II. The shrine was illegally acquired by the City and County of Honolulu in June 1942. After internment on the mainland, the priest and family returned to Hawaii in mid-December 1945. A temporary shrine was consecrated in a residence-like warehouse in McCully area of Honolulu and served as a worship site from 1946-1968. The original shrine property was returned to the shrine organization in October 1961 as a result of lengthy legal and legislative appeals. The shrine building was moved in 1963 to its present location to make way for Federal Housing Administration redevelopment. The shrine was restored from 1968-1969 at a cost of $170,000. Funds were donated entirely by the people of Hawaii. The shrine was rededicated on 22 December 1968. See also Japanese Peace Bell Hiroshima Peace Memorial Park List of Shinto shrines in the United States References External links Izumo Taishakyo Mission of Hawaii on Facebook
James L. Coke House

The James L. Coke House, also called Waipuna ('springwater' in the Hawaiian language), at 3649 Nuʻuanu Pali Drive in Honolulu, Hawaiʻi was built in 1934 for Judge James L. Coke, who had that year been reappointed Chief Justice of the Hawaii Supreme Court by U.S. President Franklin D. Roosevelt. Its architecture is significant as an example of the residential work of C.W. Dickey, the most prominent local architect of the period, and its landscaping represents the work of the preeminent landscape architect of the period, Richard Tongg. The house and grounds were added to the National Register of Historic Places in 1986. The house is not typical of Dickey's residential work, but displays fine craftsmanship and is well adapted to an indoor-outdoor lifestyle. It is a two-story, double-wall building on an L-shaped plan, with a gabled roof over one wing and a hipped roof over the other. The outside walls are of brick on the ground floor, with clapboard siding on the upper floor, both painted white. The interior floors are of ohia wood and the stairway bannister and dining room chandelier are of wrought iron. Tongg landscaped both the front yard and the back lot, which straddles Nuʻuanu Stream, during 1935–37. Among his other notable landscape designs were Andrews Outdoor Theatre at the University of Hawaiʻi, the Alexander & Baldwin Building, local residences for George W. Vanderbilt and Doris Duke, and the central concourse garden at Honolulu International Airport. References Sakamoto, Dean, ed. (2007), Hawaiian Modern: The Architecture of Vladimir Ossipoff New Haven: Honolulu Academy of Arts and Yale University Press. ISBN 978-0-300-12146-9
Telescopio Gemini Frederic C. Gillet

El Telescopio Gemini Frederick C. Gillet lleva este nombre en honor del astrónomo Frederick C. Gillet (1937-2001), uno de los pioneros en el área de la astronomía infrarroja, con grandes contribuciones a lo largo de sus más de 40 años de carrera. Entre 1979 y 1989 fue miembro del Observatorio Kitt Peak, donde alcanzó el cargo de director por un periodo. Luego, en 1983 tuvo un rol clave en el descubrimiento del fenómeno Vega, conocido como el polvoriento disco que se encuentra alrededor de la brillante estrella Vega. Esta fue la primera observación que confirmó que los planetas pueden existir alrededor de estrellas que no sean nuestro Sol. También en esa década, ayudó a la NASA, donde cooperó con los proyectos SIRTF y SOFIA. Ya en 1984 recibió la medalla científica de logro excepcional otorgada por la NASA por su trabajo en satélites astronómicos destinados al estudio de la radiación infrarroja. El Dr. Gillett tuvo una larga asociación con el Observatorio Nacional de Astronomía Óptica (en inglés, NOAO, National Optical Astronomical Observatory) en Tucson. Allí fue asociado con el éxito del IRAS (Infrared Astronomy Satellite), considerado un hito en la historia de la astronomía infrarroja. A lo largo de su trayectoria realizó también diversos estudios de Saturno, Urano y Neptuno, además de observaciones de la Vía Láctea y regiones de formación estelar en la galaxia, pero sin duda su mayor contribución a esta ciencia fue el hecho de que fue uno de los visionarios que participaron en la construcción del Observatorio Gemini, ya que estaba seguro de que el diseño de estos telescopios gemelos de 81 dm, ubicados en ambos hemisferios del planeta, serían una contribución científica a la astronomía del siglo XXI. Su gran dedicación en el desarrollo de este Observatorio, llevó a que se nombrara en su honor a uno de los telescopios gemelos: Gemini Norte, ubicado en Mauna Kea, el cual pasó a nombrarse “Telescopio Gemini Frederick C. Gillett” en una ceremonia realizada el 13 de noviembre de 2002, un año después de su muerte en el mes de abril cuando falleció a los 64 años en el Centro Médico de la Universidad de Washington a causa de un extraño desorden en la médula ósea. Véase también Lista de los mayores telescopios reflectores ópticos
Jessie Eyman–Wilma Judson House

The Jessie Eyman–Wilma Judson House at 3114 Paty Drive in Honolulu, Hawaiʻi, was one of the earliest residences designed by C.W. Dickey in his "Hawaiian style" after he finally returned to the islands for good in 1925. It was built in 1926 for Jessie Eyman and Wilma Judson, two nurses who arrived from Illinois in 1925. The house was added to the National Register of Historic Places in 1986. The house sits on a sharply triangular hillside lot overlooking Manoa Valley at the intersection of Alani Drive (below) and Paty Drive (above, formerly Dillingham Drive). Its "Hawaiian style" architecture includes Dickey's trademark double-pitched hip roof with overhanging eaves, ample windows, and an enclosed lanai at the south-facing entrance. The single-story house, one-room deep, with board-and-batten siding, wraps around an open courtyard in the rear. One wing off the living room contains two bedrooms and a bath. The dining room and kitchen occupy the right rear wing, near a maid's quarters and a garage on the south side. The original owners lived in the house until 1940, when Judson sold her share to Eyman, who sold the house in 1943. As nurses, they set up the first Physicians Telephone Exchange in the Territory. Judson also worked many years for Dr. Forrest Joy Pinkerton, who founded the Blood Bank of Hawaiʻi and the Pan-Pacific Surgical Association. Eyman managed the Mabel Smyth Memorial Building from the time it was built in 1941 until she retired in 1952. References
Messstation Mauna Loa

Die Messstation Mauna Loa ist eine meteorologische Forschungsstation in 3397 Metern Höhe auf dem Vulkan Mauna Loa auf Hawaii. Sie gehört zum Earth System Research Laboratory (ESRL) des Office of Oceanic and Atmospheric Research (OAR), einer Abteilung der National Oceanic and Atmospheric Administration (NOAA) der Vereinigten Staaten. Um herauszufinden, welchen Einfluss der Mensch auf die Zusammensetzung der Atmosphäre hat und wie stark die Emissionen des Treibhausgases Kohlenstoffdioxid (CO2) sind, wird in der Messstation seit 1958 der CO2-Gehalt der Luft gemessen. Die daraus entstandene Messreihe, die nach dem maßgeblich beteiligten Forscher Charles David Keeling benannte Keeling-Kurve, ist die längste kontinuierliche Aufzeichnung der CO2-Konzentration in der Atmosphäre. Die Messungen dokumentieren den steigenden Gehalt an CO2 in der Atmosphäre durch die Verbrennung fossiler Kohlenwasserstoffe. Auf vier 7 m und einem 27 m hohen Turm mit Lufteinlass werden stündlich vier Luftproben der Atmosphäre entnommen. Die stündlichen Durchschnittswerte des CO2-Gehalts, der Windgeschwindigkeit und Windrichtung bilden die Grundlage für die weitere Auswertung. Um den täglichen Durchschnitt zu ermitteln, werden die Daten von mindestens sechs aufeinander folgenden Stunden benötigt. Die Daten bilden eine Grundlage für die Entwicklung von Klimaszenarien durch Modelle. Die Lage der Messstation auf Hawaii ist für atmosphärische Messungen besonders geeignet, da die Luft in der Umgebung kaum durch lokale Einflüsse der Vegetation oder der Menschen beeinträchtigt wird. Seit Beginn der Messreihe, 1958, hat sich an der Ausrüstung und den Methoden im Wesentlichen nichts verändert. Weblinks Offizielle Website des Observatoriums Mauna Loa
Observatoire du Mauna Loa

L'observatoire du Mauna Loa, en anglais Mauna Loa Observatory (MLO), est un observatoire atmosphérique des États-Unis situé à Hawaï, construit en 1956 à 3 397 mètres d'altitude sur le Mauna Loa, le plus haut volcan de Big Island. Activités scientifiques Depuis 1957 et de façon continue depuis 1958, il mesure la teneur en dioxyde de carbone dans l'atmosphère, données utilisées pour obtenir la courbe de Keeling. Géré par la National Oceanic and Atmospheric Administration, il est appuyé par un bureau situé à Hilo, ouvert en 1959. Notes et références Voir aussi Bibliographie (en) Forrest M. Mims, Hawai‘i’s Mauna Loa Observatory: Fifty Years of Monitoring the Atmosphere, University of Hawaii Press, novembre 2011 (ISBN 978-0-8248-3718-1, DOI 10.1515/9780824837181, lire en ligne). Articles connexes Observatoire solaire du Mauna Loa Observatoire de Haute Altitude (en) Base Martin-de-Viviès sur l'Île Amsterdam, qui mesure aussi depuis 1980 la teneur en CO2. Liens externes Portail des sciences Portail d’Hawaï
Mauna Loa Observatorium

Het Mauna Loa Observatorium (MLO) is een observatiestation voor de aardatmosfeer op Mauna Loa, een vulkaan op het eiland Hawaï. Het observatorium is gelegen op 3397 meter hoogte, op de helling van de vulkaan. Sedert 1956 verzamelt het gegevens over allerlei veranderingen in de atmosfeer, aanvankelijk onder leiding van Charles Keeling, nadien van zijn zoon Ralph en later Elmer Robinson. Maar het centrum is vooral bekend om zijn ononderbroken meting van het gehalte koolstofdioxide (CO2) in de atmosfeer. Soms wordt hier ook naar verwezen als de Keelingcurve. Het observatorium maakt deel uit van het Earth System Research Laboratory, een onderdeel van de National Oceanic and Atmospheric Administration (NOAA). Volgens dit agentschap is Mauna Loa het oudste continue CO2-waarnemingsstation op aarde, en wereldwijd de bekendste maatstaf voor het meten van het gas. Op dezelfde locatie als het MLO bevinden zich ook het Mauna Loa Solar Observatorium en AmiBA (meten van kosmische achtergrondstraling). Elders op Hawaï ligt het astronomisch Mauna Kea-observatorium. Mauna Loa werd oorspronkelijk als locatie gekozen vanwege de afstand tot het continent, de hoogteligging boven de inversielaag, en omdat er al een ruwe toegangsweg bestond. Soms worden de metingen verstoord door lokale vulkaanemissies, maar die worden dan gecorrigeerd. CO2-metingen De metingen op Mauna Loa laten in de 21e eeuw een uitgesproken stijging van het CO2-gehalte zien. Sedert 2015 is de symbolische grens van 400 ppm CO2 overschreden. Gelijkaardige metingen worden uitgevoerd in het Cape Grim Baseline Air Pollution Station (Australië). Het Earth System Research Laboratory verzamelt en integreert ook metingen van over de hele wereld. Zie ook Broeikaseffect Broeikasgas CO2-metingen (1750-heden) Externe link website Mauna Loa Observatorium
Observatório Mauna Loa

O Observatório Mauna Loa (MLO) é uma estação de referência atmosférica em Mauna Loa, na ilha do Havaí, localizada no estado americano do Havaí. O observatório Desde 1958, inicialmente sob a direção de Charles Keeling, seguido por seu filho Ralph e posteriormente Elmer Robinson, o Observatório Mauna Loa (Mauna Loa Observatory em inglês, ou MLO) monitora e coleta dados relativos às mudanças atmosféricas, e é conhecido especialmente pelo monitoramento contínuo do dióxido de carbono atmosférico (CO2), que às vezes é referido como a Curva de Keeling. O observatório está subordinado ao Laboratório de Pesquisa do Sistema Terrestre, que faz parte da Administração Oceânica e Atmosférica Nacional (NOAA). De acordo com a NOAA, Mauna Loa é a estação de monitoramento contínuo de CO 2 mais antiga do mundo e o principal local de referência do mundo para medição do gás. As mais recentes observações das concentrações de CO2 do MLO podem ser encontradas em sites da web junto com dados de outros sites e tendências em Mauna Loa. Os níveis de MLO podem ser comparados com outros sites na rede de monitoramento global. O MLO tem atividades em cinco locais na Ilha Grande. O principal local de observação está localizado a 3397 metros de altura na encosta norte de Mauna Loa cerca de 5 km (3 mi) ao norte do cume Mokuaweoweo . O Observatório Solar Mauna Loa compartilha este site. A administração e alguns processamentos de dados são feitos no escritório de Hilo, Havaí. Kulani Mauka é um local de coleta de chuva. Cape Kumukahi é um local de amostra de frasco localizado no ponto mais oriental do Havaí. No aeroporto de Hilo, instrumentos transportados por balão são preparados e lançados para medir o ozônio da superfície até normalmente mais de 30 quilômetros (19 mi) de altura. O local do observatório também é um lar temporário para um observatório cósmico de fundo de microondas chamado AMiBA. Mauna Loa foi originalmente escolhida como local de monitoramento porque, localizada longe de qualquer continente, o ar amostrado lá é uma boa média para o Pacífico central. Ver também Observatórios Mauna Kea Referências Ligações externas Site oficial do NOAA Mauna Loa Observatory Divisão de Monitoramento Global, Boulder, CO, EUA Concentrações mundiais de dióxido de carbono - em tempo real
Погодная обсерватория на Мауна-Лоа

Погодная обсерватория на Мауна-Лоа (англ. Mauna Loa Observatory (MLO)) — атмосферная станция у вершины вулкана Мауна-Лоа, на острове Гавайи, США. Обсерватория С 1956 года обсерватория на Мауна-Лоа осуществляет мониторинг и сбор данных, касающихся атмосферных изменений. Особенно важного для непрерывного мониторинга атмосферного углекислого газа (CO2), называемой Кривой Килинга. Обсерватория является частью Национального управления океанических и атмосферных исследований (NOAA). По данным НОАА, Мауна-Лоа является старейшей в мире непрерывно CO2 ПЦН, и в мире основного критерия сайте для измерения газа. Последние наблюдения CO2 концентрации можно найти на веб-сайтах вместе с данными с других сайтов , а также тенденций на Мауна-Лоа. МЗО уровни можно сравнить с другими сайтами в глобальной сети мониторинга. Обсерватория находится на высоте 3397 метров над уровнем моря на Северном склоне Мауна-Лоа, примерно в 6 км к северу от кальдеры вулкана Мауна-Лоа. Мауна-Лоа была выбрана в качестве площадки для мониторинга, потому что находится наиболее далеко от любого континента, посреди Тихого океана. Она расположена выше инверсионного слоя, вдали от загрязнений. Возможное влияние от местных вулканических источников удаляется из полученных данных. Филиалы Администрация и некоторые данные обработки проводятся в городе Хило, Гавайи офис. Куланами Маука — место для сбора дождевой воды. Мыс Kumukahi пример сайта фляга находится в самой восточной части Гавайи. В аэропорту хило, еженедельно запускаются шары-зонды для измерения озона на высоты более 30 км. На обсерватории также размещён космический микроволновый фоновый детектор под названием AMiBA. См. также Углекислый газ в атмосфере Земли Обсерватории на вулкане Мауна Кеа, остров Гавайи Гавайская вулканическая обсерватория Примечания Ссылки НОАА Мауна-Лоа обсерватория Архивная копия от 6 ноября 2010 на Wayback Machine официальный сайт Глобальный Отдел мониторинга, Боулдер, Колорадо, США Архивная копия от 17 декабря 2013 на Wayback Machine Мировой концентрации углекислого газа в режиме реального времени Архивная копия от 13 февраля 2021 на Wayback Machine
John Guild House

The John Guild House, now known as Manoa Valley Inn, at 2001 Vancouver Drive in Honolulu, Hawaii, was purchased in 1919 by John Guild, a Honolulu businessman. It had been built four years earlier by Iowa lumber dealer Milton Moore and has been refurbished and restored several times over its lifespan. It was listed on the National Register of Historic Places in 2002. The house was purchased in the 1980s by Honolulu businessman Rick Ralston (the founder of Crazy Shirts), who restored it in 1982 for use as a bed and breakfast under the name John Guild Inn, later Manoa Valley Inn, the name under which it still operates. In 1990, the Nakamitsu Corporation purchased and further refurbished it. The three-story gabled cottage near the campus of the University of Hawaii at Manoa contains eight guest rooms furnished with fine antiques. Among its architectural features are multiple extended gables with decorative buttresses, a porte-cochere in the same style on the valley side of the house, and a broad, sheltered lanai with a view over the city on the sea side of the house. In 2007, the current owner and operator of the Manoa Valley Inn put it up for sale at $4.2 million for the half-acre lot and 4,424-square-foot (411.0 m2) house. She decided to sell it after the external chimney was badly damaged in the earthquake of 15 October 2006. The rest of the house was undamaged. References Sandler, Rob, Julie Mehta, and Frank S. Haines (2008). Architecture in Hawai‘i: A Chronological Survey, new edition. Honolulu: Mutual Publishing. ISBN 978-1-56647-873-1 External links Manoa Valley Inn
KKCR

KKCR (90.9 FM) is a community radio station broadcasting a variety format including Hawaiian, jazz, blues, R&B, rock, reggae, classical and world artists as well as locally produced talk programs. Licensed to the Kekahu Foundation in Hanalei, Hawaii, United States, the station serves the island of Kauaʻi and parts of Oahu. The station is owned by the Kekahu Foundation, Inc. The idea for KKCR originated in the late '80s. Janet Friend, Roy Richardson, Richard Fernandez, Jon and Lorraine Scott, and other Island residents decided to start a radio station that would serve Island residents, withstand extreme weather conditions and provide emergency information to isolated residents. The station provides one of the primary Emergency Alert System signals on Kauaʻi. Repeaters Translators and boosters KKCR also broadcasts on radio station KAQA 91.9 MHz Kauaʻi, KAQA's FM booster 92.7 MHz via translator K224CQ in Anahola, Hawaii and 88.9 MHz via translator K205FM in Honolulu, Hawaii. See also List of community radio stations in the United States References External links Official website Facility details for Facility ID 33827 (KKCR) in the FCC Licensing and Management System KKCR in Nielsen Audio's FM station database Video tour of KKCR studios during its construction in 1997 on YouTube Video of maintenance of transmitter atop Mt. Kahili via helicopter on YouTube ——— Facility details for Facility ID 33826 (KAQA) in the FCC Licensing and Management System KAQA in Nielsen Audio's FM station database Facility details for Facility ID 84395 (K205FM) in the FCC Licensing and Management System K205FM at FCCdata.org Facility details for Facility ID 146232 (K224CQ) in the FCC Licensing and Management System K224CQ at FCCdata.org
Ka'ena Point Space Force Station

Ka'ena Point Space Force Station is a United States Space Force installation in Ka'ena Point on the island of Oahu in Hawaii. It is a remote tracking station of the Satellite Control Network responsible for tracking satellites in orbit, many of which support the United States Department of Defense, receiving and processing data and in turn, enabling control of satellites by relaying commands from control centers. The station originally opened in 1959 to support the Corona reconnaissance program. Detachment 3, 21st Space Operations Squadron, part of Space Delta 6, operates Hawaii Tracking Station on the site. It was constructed in 1959, one of three built that year. The facility is placed near the westernmost point of the island of Oahu, atop a 1,500-foot (460 m) high ridge. The two radomes are locally known as the "golf balls", and are a popular landmark for fishing vessels in the surrounding waters. Yokohama Bay State Park is at the base of the ridge, with a hiking trail that goes to the point and around to the northern side of the ridge, to Mokuleia Beach. The station roadways provide access to state hiking and hunting trails, as well as a camping site about 10 miles (16 km) inland called Peacock Flats by permit only. Permits to enter through the station to hike, hunt, or camp on the surrounding State lands can be obtained from the Hawaii Department of Land and Natural Resources in downtown Honolulu. On 16 June 2021, it was renamed from Ka'ena Point Satellite Tracking Station to Ka'ena Point Space Force Station. References External links Permission form Historic American Engineering Record (HAER) documentation, filed under Ka'ena Point, Wai'anae Mountains above Keawaula Bay, Waialua, Honolulu County, HI: HAER No. HI-97, "Ka'ena Point Satellite Tracking Station", 10 photos, 21 data pages, 2 photo caption pages HAER No. HI-97-A, "Ka'ena Point Satellite Tracking Station, Building 20", 13 photos, 2 photo caption pages HAER No. HI-97-B, "Ka'ena Point Satellite Tracking Station, Building 14111", 9 photos, 1 photo caption page HAER No. HI-97-C, "Ka'ena Point Satellite Tracking Station, Building 21", 5 photos, 1 photo caption page HAER No. HI-97-D, "Ka'ena Point Satellite Tracking Station, Building 11", 8 photos, 6 data pages, 1 photo caption page HAER No. HI-97-E, "Ka'ena Point Satellite Tracking Station, Building 35", 14 photos, 8 data pages, 2 photo caption pages HAER No. HI-97-F, "Ka'ena Point Satellite Tracking Station, Building 39005", 12 photos, 7 data pages, 2 photo caption pages HAER No. HI-97-G, "Ka'ena Point Satellite Tracking Station, Building 39006", 11 photos, 7 data pages, 2 photo caption pages