Difference between revisions 1220480 and 1229608 on enwikiversity[[Image:Brorfelde Schmidt Telescope.jpg|thumb|right|200px|The Schmidt Telescope at the former Brorfelde Observatory is now used by amateur astronomers. Credit: [[commons:User:Moeng|Mogens Engelund]].]] {{complete}} A '''radiation telescope''' is an instrument designed to collect and focus radiation so as to make distant sources appear nearer. {{experimental}} {{primary}} {{secondary}} {{tertiary}} {{research}} (contracted; show full)|location=San Francisco, California |month=April 2, |year=2013 |url=http://en.wiktionary.org/wiki/radiotelescopy |pdf= |accessdate=2013-07-21 }}</ref> is called '''radiotelescopy'''. =Entities=⏎ ⏎ =Sources= [[Image:Horizontal cyclotron with glowing beam.jpg|thumb|center|300px|This image shows a beam of accelerated ions (perhaps protons or deuterons) escaping the accelerator and ionizing the surrounding air causing a blue glow. Credit: Lawrence Berkely National Laboratory.]] [[Image:Synchrotron light.jpeg|thumb|right|200px|The image shows the blue glow given off by the synchrotron beam from the National Synchrotron Light Source. Credit: NSLS, Brookhaven National Laboratory.]] The image above shows a blue glow in the surrounding air from emitted cyclotron particulate radiation. At right is an image that shows the blue glow resulting from a beam of relativistic electrons as they slow down. This deceleration produces synchrotron light out of the beam line of the National Synchrotron Light Source. {{clear}} =Objects= =Strong forces= =Electromagnetics= =Weak forces= =Continua= =Emissions= =Absorptions=⏎ ⏎ =Bands= [[Image:Rosetta.jpg|thumb|right|200px|This is a 3D model of the Rosetta Spacecraft. The individual scientific payloads are highlighted in different colours. Credit: [[w:User:IanShazell|IanShazell]].]] (contracted; show full)|year=2013 |url=https://en.wikipedia.org/wiki/Liquid_mirror_telescope |accessdate=2014-01-03 }}</ref> A "telescope with a liquid metal mirror can only be used [as a] zenith telescope that looks straight up".<ref name=LiquidMirrorTelescope/> {{clear}} =Rocky-object telescopes=⏎ ⏎ =Hydrogen telescopes= [[Image:Solarborg.jpg|right|thumb|200px|Here is an example of an amateur solar telescope equipped with a hydrogen-alpha filter system. Credit: .]] "In the field of [[amateur astronomy]] ... Amateurs use ... hydrogen-alpha filter systems".<ref name=SolarTelescope>{{ cite web |title=Solar telescope, In: ''Wikipedia'' |publisher=Wikimedia Foundation, Inc |location=San Francisco, California |month=December 30, |year=2013 |url=https://en.wikipedia.org/wiki/Solar_telescope |accessdate=2014-01-03 }}</ref> {{clear}} =Ions= =Compounds=⏎ ⏎ =Alloys= [[Image:Cloudcroft Observatory.jpg|thumb|right|200px|The image shows the dome of the NASA Orbital Debris Observatory near Cloudcroft, New Mexico. Credit: NASA.]] [[Image:CCD_Debris_Telescope.png|thumb|left|200px|This image shows the CCD Debris Telescope that is under the NODO dome. Credit: ]] "The NASA-LMT was 3 m (9.8 ft) aperture liquid mirror telescope located in NODO's main dome. It consisted of a 3 m diameter parabolic dish that held 4 U.S. gallons (15 l) of a highly reflective liquid metal, mercury, spinning at a rate of 10 rpm, with sensors mounted above on a fixed structure. Due to the primary mirror's material, the NASA-LMT was configured as a zenith telescope. Using 20 narrowband filters, it cataloged space debris in Earth's orbit."<ref name=NASAOrbitalDebrisObservatory>{{ cite web |title=NASA Orbital Debris Observatory, In: ''Wikipedia'' |publisher=Wikimedia Foundation, Inc |location=San Francisco, California |month=May 6, |year=2013 |url=https://en.wikipedia.org/wiki/NASA_Orbital_Debris_Observatory |accessdate=2014-01-03 }}</ref> "The 32 cm (13 in) CCD Debris Telescope (CDT) was a portable Schmidt camera equipped with a 512×512 pixel charge-coupled device (CCD) sensor. It operated at NODO from October of 1997 until December of 2001, and was used to characterize debris at or near geosynchronous orbit."<ref name=NASAOrbitalDebrisObservatory/> {{clear}} =Atmospheres= =Materials=⏎ ⏎ =Meteorites= [[Image:Carancas Meteorite 2.jpg|thumb|right|200px|The image contains a 27.70 g fragment of the Carancas meteorite fall. The scale cube is 1 cm<sup>3</sup>. Credit: Meteorite Recon.]] (contracted; show full)|year=2013 |url=http://en.wikipedia.org/wiki/Large_Binocular_Telescope |accessdate=2013-07-02 }}</ref> "The first image taken [shown at right] combined ultraviolet and green light, and emphasizes the clumpy regions of newly formed hot stars in the spiral arms."<ref name=LargeBinocularTelescope/> {{clear}} =Chemistry=⏎ ⏎ =Geography= [[Image:VERITAS array.jpg|thumb|right|300px|VERITAS is located at the basecamp of the Smithsonian Astrophysics Observatory's Fred Lawrence Whipple Observatory (FLWO) in southern Arizona. Credit: VERITAS.]] [[Image:Aerial View of the VLTI with Tunnels Superimposed.jpg|200px|thumb|left|The four Unit Telescopes form the VLT together with the Auxiliary Telescopes. Credit: .]] (contracted; show full){{clear}} =History= [[File:TransitCircle USNO.jpg|thumb|right|200px|This is the 6-inch transit circle of the U.S. Naval Observatory. Credit: .]] The 6-inch transit circle [imaged at right] of the U.S. Naval Observatory was built by Warner and Swasey in 1898. {{clear}} =Mathematics= =Physics= =Science= =Technology=⏎ ⏎ =Apertures= "Some X-ray telescopes use coded aperture imaging. This technique uses a flat aperture grille in front of the detector, which weighs much less than any kind of focusing X-ray lens, but requires considerably more post-processing to produce an image."<ref name=XRayTelescope>{{ cite web |title=X-ray telescope, In: ''Wikipedia'' |publisher=Wikimedia Foundation, Inc |location=San Francisco, California |month=April 17, |year=2012 (contracted; show full)* [[Radiation detectors]] * [[Radiation satellites]] {{Div col end}} =References= {{reflist|2}} =Further reading=⏎ ⏎ =External links= * [http://www.ajol.info/ African Journals Online] * [http://www.bing.com/search?q=&go=&qs=n&sk=&sc=8-15&qb=1&FORM=AXRE Bing Advanced search] * [http://books.google.com/ Google Books] * [http://scholar.google.com/advanced_scholar_search?hl=en&lr= Google scholar Advanced Scholar Search] * [http://www.iau.org/ International Astronomical Union] * [http://www.jstor.org/ JSTOR] * [http://www.lycos.com/ Lycos search] (contracted; show full)* [http://search.yahoo.com/web/advanced Yahoo Advanced Web Search] <!-- footer templates --> {{Astronomy resources}} {{Principles of radiation astronomy}} {{Technology resources}} {{Research project}} {{Sisterlinks|Radiation telescope s}} {{Sisterlinks|Telescopes}} <!-- categories --> [[Category:Astronomy]] [[Category:Astronomy Project]] [[Category:Original research]] [[Category:Physics and Astronomy]] [[Category:Research]] [[Category:Research projects]] [[Category:Resources last modified in JanuarySeptember 2014]] [[Category:Technology]] <!-- interlanguage links --> All content in the above text box is licensed under the Creative Commons Attribution-ShareAlike license Version 4 and was originally sourced from https://en.wikiversity.org/w/index.php?diff=prev&oldid=1229608.
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