Субміліметрова антенна система
The name shown is in uk. The article below is in English and is not a translation.
≈ 3 min read
Names in other languages
- УкраїнськаСубміліметрова антенна системаSub-Millimeter Array, SMA
- eoSubmilimetra Teleskoparo
- ltSubmilimetrinis masyvas
- caSubmillimeter Array
- DeutschSubmillimeter Array
- EnglishSubmillimeter Array
- FrançaisSubmillimeter Array
- ItalianoSubmillimeter Array
- lbSubmillimeter Array
- nbSubmillimeter Array
- PortuguêsSubmillimeter Array
- slSubmillimeter ArraySubmilimetrsko polje, Submilimetrski antenski sistem
- فارسیآرایه زیرمیلیمتریSMA
- 한국어서브밀리미터 집합체서브미리메터 집합체, 서브미리파 집합체, 서브밀리미터 어레이, 서브밀리파 집합체
- 中文次毫米波陣列望遠鏡
- 简体中文次毫米波阵列望远镜
- 繁體中文次毫米波陣列望遠鏡
- 中文次毫米波陣列望遠鏡
- 日本語サブミリ波干渉計Submillimeter Array
Article bodies are English and are not machine-translated. A name in another language is not a translation of the article.
The Submillimeter Array (SMA) consists of eight diameter radio telescopes arranged as an interferometer for submillimeter wavelength observations. It is the first purpose-built submillimeter interferometer, constructed after successful interferometry experiments using the pre-existing James Clerk Maxwell Telescope and Caltech Submillimeter Observatory (now decommissioned) as an interferometer. All three of these observatories are located at Mauna Kea Observatory on Mauna Kea, Hawaii, and have been operated together as a ten element interferometer in the 230 and 345 GHz bands (eSMA, for extended Submillimeter Array). The baseline lengths presently in use range from . The radio frequencies accessible to this telescope range from which includes rotational transitions of dozens of molecular species as well as continuum emission from interstellar dust grains. Although the array is capable of operating both day and night, most of the observations take place at nighttime when the atmospheric phase stability is best. The SMA is jointly operated by the Smithsonian Astrophysical Observatory (SAO) and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA).
The Submillimeter Array (SMA) consists of eight diameter radio telescopes arranged as an interferometer for submillimeter wavelength observations. It is the first purpose-built submillimeter interferometer, constructed after successful interferometry experiments using the pre-existing James Clerk Maxwell Telescope and Caltech Submillimeter Observatory (now decommissioned) as an interferometer. All three of these observatories are located at Mauna Kea Observatory on Mauna Kea, Hawaii, and have been operated together as a ten element interferometer in the 230 and 345 GHz bands (eSMA, for extended Submillimeter Array). The baseline lengths presently in use range from . The radio frequencies accessible to this telescope range from which includes rotational transitions of dozens of molecular species as well as continuum emission from interstellar dust grains. Although the array is capable of operating both day and night, most of the observations take place at nighttime when the atmospheric phase stability is best. The SMA is jointly operated by the Smithsonian Astrophysical Observatory (SAO) and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA).
Text derived from https://en.wikipedia.org/w/index.php?oldid=1369307263 under CC BY-SA 4.0; modifications have been made.