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http://dbpedia.org/ontology/abstract The Global Oscillation Network Group (GONGThe Global Oscillation Network Group (GONG) is a worldwide network of six identical telescopes, designed to have 24/7 observations of the Sun. The network serves multiple purposes, including the provision of operation data for use in space weather prediction, and the study of solar internal structure and dynamics using helioseismology. Deployed in 1995, GONG is a set of six observing systems geographically distributed around the Earth so that the Sun can be observed as continuously as possible. The six observatories are the Teide Observatory (Canary Islands), the Learmonth Solar Observatory (Western Australia), the Big Bear Solar Observatory (California), the Mauna Loa Solar Observatory (Hawaii), the Udaipur Solar Observatory (India) and the Cerro Tololo Inter-American Observatory (Chile). With these sites, GONG typically can observe the Sun 91% of the time, 24/7. GONG was constructed to provide observations for helioseismology, which aims to understand the solar interior by analyzing the sound waves that are trapped in it. In 2001, the original GONG detectors were upgraded to 1000 x 1000 pixels and continuous magnetograms were implemented, and the new system is known as GONG++. While GONG still provides helioseismology data, it now also provides full-disk solar magnetic field maps (magnetograms) every minute and full-disk images of the Sun in the wavelength of the Hydrogen–α (Hα) spectral line every 20 seconds. These data products are used for research into the solar magnetic field and chromosphere but are also essential inputs into forecasts of space weather. The NOAA Space Weather Prediction Center (SWPC), the US Airforce 557th Weather Wing, and the NASA Community Coordinated Modeling Center (CCMC) all use GONG data to predict space weather conditions. The GONG Project is managed by the , which is operated by AURA, Inc. under a cooperative agreement with the National Science Foundation. GONG has been in operation since 1995 and is aging rapidly. To replace it, NSO is proposing to design and build a next-generation Ground-based solar Observing Network, provisionally named ngGONG.rving Network, provisionally named ngGONG. , 全球日震觀測網 (Global Oscillation Network Group,全球日震觀測網 (Global Oscillation Network Group,GONG) 是一個以日震學研究太陽內部結構和動力學的社群基礎計畫。 涉及六個太陽觀測站,以實現幾乎不間斷觀測太陽的目的。這六個天文台是 (加納利群島)、 (西澳大利亞)、大熊湖太陽天文台 (加利福尼亞州)、茂納羅亞太陽天文台 (夏威夷)、 (印度)和托洛洛山美洲際天文台 (智利)。在2001年,原始的GONG檢測器升級為1000 X 1000畫素,並且加入了連續的磁強圖,新的系統稱為GONG++。 GONG計畫由國家太陽天文台管理,根據與國家自然科學基金會的合作協定,由AURA公司操作。G計畫由國家太陽天文台管理,根據與國家自然科學基金會的合作協定,由AURA公司操作。
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rdfs:comment 全球日震觀測網 (Global Oscillation Network Group,全球日震觀測網 (Global Oscillation Network Group,GONG) 是一個以日震學研究太陽內部結構和動力學的社群基礎計畫。 涉及六個太陽觀測站,以實現幾乎不間斷觀測太陽的目的。這六個天文台是 (加納利群島)、 (西澳大利亞)、大熊湖太陽天文台 (加利福尼亞州)、茂納羅亞太陽天文台 (夏威夷)、 (印度)和托洛洛山美洲際天文台 (智利)。在2001年,原始的GONG檢測器升級為1000 X 1000畫素,並且加入了連續的磁強圖,新的系統稱為GONG++。 GONG計畫由國家太陽天文台管理,根據與國家自然科學基金會的合作協定,由AURA公司操作。G計畫由國家太陽天文台管理,根據與國家自然科學基金會的合作協定,由AURA公司操作。 , The Global Oscillation Network Group (GONGThe Global Oscillation Network Group (GONG) is a worldwide network of six identical telescopes, designed to have 24/7 observations of the Sun. The network serves multiple purposes, including the provision of operation data for use in space weather prediction, and the study of solar internal structure and dynamics using helioseismology.ucture and dynamics using helioseismology.
rdfs:label Global Oscillations Network Group , 全球日震觀測網
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