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1. The Very Large Telescope Project
... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/projects/vlt/ -- 8.6 Кб -- 03.04.2006
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2. DOK-2 Results Page
The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/auroral/dok2.htm -- 9.9 Кб -- 28.11.1996
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/auroral/dok2.htm -- 9.9 Кб -- 28.11.1996
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3. Space Telescope Science Institute
STScI . ... What is STScI . ... Hubble Heritage Project . ... Research . Research Staff Directory . Journal Clubs and Research Groups . Colloquia . ... Hubble Fellowships . ... Youth for Astronomy and Engineering . ... Engineering Technology Colloquia . ... Operates the science program for the Hubble Space Telescope and will conduct the science and mission operations for the James Webb Space Telescope and supports other astronomy programs and conducts world-class scientific research. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute -- 17.7 Кб -- 09.04.2016
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4. Proposed Facility
... Clearly, what we need is big telescopes with high resolution spectrographs, to get good data on QSO absorption-lines. With bigger and better telescopes, you could measure the clustering and 3D distribution of gas in the early universe, by looking at lots of faint QSOs in the same parts of the sky. ... With the high resolutions made possible by big telescopes, you could look at the internal velocity structure of the absorbing clouds. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node25.html -- 3.9 Кб -- 02.10.2012
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