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- ...ame ultraviolet comes from [[latin|Latin]] ''ultra'' meaning beyond, i.e., ultraviolet has a higher frequency than violet in the [[Electromagnetic spectrum|spectr |Near Ultraviolet, Ultraviolet A2 KB (347 words) - 04:54, 14 March 2024
- 132 bytes (16 words) - 14:07, 25 January 2009
- ...an astronomical [[observatory]] [[satellite]] primarily designed to take [[ultraviolet]] [[Electromagnetic spectrum|spectra]]. The satellite was a collaborative p <caption><br>'''International Ultraviolet Explorer (IUE)'''</caption>7 KB (1,076 words) - 09:16, 6 March 2024
- Auto-populated based on [[Special:WhatLinksHere/Ultraviolet]]. Needs checking by a human. {{r|Hopkins Ultraviolet Telescope}}2 KB (206 words) - 15:53, 4 April 2024
- The '''Hopkins Ultraviolet Telescope''' (HUT) was one of three [[ultraviolet]] instruments of the [[ASTRO-1 mission]] flown on the [[space shuttle]] [[S [[Image:Hut2.jpg|frame|center|Hopkins Ultraviolet Telescope]]733 bytes (98 words) - 15:26, 3 November 2007
- 12 bytes (1 word) - 15:26, 3 November 2007
- Space telescope designed to make spectroscopic observations in the far-ultraviolet region of the electromagnetic spectrum, flown into orbit on the Space Shutt234 bytes (30 words) - 06:11, 12 September 2009
- 12 bytes (1 word) - 20:11, 3 November 2007
- An astronomical [[satellite]] designed primarily to observe [[ultraviolet]] spectra.120 bytes (12 words) - 18:49, 29 November 2008
- {{dambigbox|the Wisconsin Ultraviolet Photo-Polarimeter Experiment|Wisconsin}} ...onsin Ultraviolet Photo-Polarimeter Experiment''' WUPPE was one of three [[ultraviolet]] [[telescope|telescopes]] on the [[ASTRO-1 mission]] flown on the [[space3 KB (427 words) - 13:04, 9 August 2023
- Auto-populated based on [[Special:WhatLinksHere/Hopkins Ultraviolet Telescope]]. Needs checking by a human. {{r|Ultraviolet}}446 bytes (56 words) - 17:16, 11 January 2010
- 105 bytes (11 words) - 23:04, 12 February 2010
- 12 bytes (1 word) - 10:28, 16 November 2007
- <noinclude>{{Subpages}}</noinclude>One of three ultraviolet telescopes on the ASTRO-1 mission flown on the space shuttle Columbia durin152 bytes (20 words) - 10:18, 13 October 2008
- Auto-populated based on [[Special:WhatLinksHere/Wisconsin Ultraviolet Photo-Polarimeter Experiment]]. Needs checking by a human. {{r|Ultraviolet}}467 bytes (57 words) - 21:42, 11 January 2010
Page text matches
- The '''Hopkins Ultraviolet Telescope''' (HUT) was one of three [[ultraviolet]] instruments of the [[ASTRO-1 mission]] flown on the [[space shuttle]] [[S [[Image:Hut2.jpg|frame|center|Hopkins Ultraviolet Telescope]]733 bytes (98 words) - 15:26, 3 November 2007
- An astronomical [[satellite]] designed primarily to observe [[ultraviolet]] spectra.120 bytes (12 words) - 18:49, 29 November 2008
- An orbiting [[ultraviolet]] space [[telescope]] that was launched on April 28, 2003.120 bytes (13 words) - 15:36, 6 July 2008
- ...ame ultraviolet comes from [[latin|Latin]] ''ultra'' meaning beyond, i.e., ultraviolet has a higher frequency than violet in the [[Electromagnetic spectrum|spectr |Near Ultraviolet, Ultraviolet A2 KB (347 words) - 04:54, 14 March 2024
- {{r|Ultraviolet|Ultraviolet light}}492 bytes (55 words) - 18:51, 18 May 2010
- Auto-populated based on [[Special:WhatLinksHere/Wisconsin Ultraviolet Photo-Polarimeter Experiment]]. Needs checking by a human. {{r|Ultraviolet}}467 bytes (57 words) - 21:42, 11 January 2010
- Auto-populated based on [[Special:WhatLinksHere/Hopkins Ultraviolet Telescope]]. Needs checking by a human. {{r|Ultraviolet}}446 bytes (56 words) - 17:16, 11 January 2010
- <noinclude>{{Subpages}}</noinclude>One of three ultraviolet telescopes on the ASTRO-1 mission flown on the space shuttle Columbia durin152 bytes (20 words) - 10:18, 13 October 2008
- Auto-populated based on [[Special:WhatLinksHere/Ultraviolet]]. Needs checking by a human. {{r|Hopkins Ultraviolet Telescope}}2 KB (206 words) - 15:53, 4 April 2024
- ...several forms, required for normal growth of teeth and bones, produced by ultraviolet irradiation and sterols found in milk, fish, and eggs.210 bytes (29 words) - 22:52, 8 September 2009
- {{r|Ultraviolet}} {{r|Wisconsin Ultraviolet Photo-Polarimeter Experiment}}990 bytes (128 words) - 20:51, 11 January 2010
- {{rpl|Wisconsin Ultraviolet Photo-Polarimeter Experiment}}195 bytes (23 words) - 13:01, 9 August 2023
- ...ere, directly above the mesosphere and directly below the exosphere, where ultraviolet radiation causes ionization and auroras also occur.203 bytes (26 words) - 00:40, 12 September 2009
- Space telescope designed to make spectroscopic observations in the far-ultraviolet region of the electromagnetic spectrum, flown into orbit on the Space Shutt234 bytes (30 words) - 06:11, 12 September 2009
- ...ing systems, to aim an optical system at a source of infrared, visible, or ultraviolet light, and follow it for purposes of observation or weapons guidance263 bytes (38 words) - 00:30, 24 August 2009
- ...d by an object, typically within the [[infrared light|infrared]] through [[ultraviolet]] wavelength range, and compare it to spectral signatures of known objects355 bytes (43 words) - 04:22, 27 December 2008
- ...patterns which only appear when held up to ordinary or [[ultraviolet light|ultraviolet]] [[light]]. Many banks issue new designs every few years in an effort to t1 KB (191 words) - 15:23, 28 August 2013
- {{r|Ultraviolet}} {{r|Wisconsin Ultraviolet Photo-Polarimeter Experiment}}1 KB (184 words) - 14:53, 6 April 2024
- ...wise specified, the photons are assumed to be in the visible, infrared, or ultraviolet spectra; there is no illumination of the target atoms as in [[atomic fluore354 bytes (54 words) - 20:28, 18 July 2010
- {{r|Ultraviolet}}339 bytes (36 words) - 20:36, 28 June 2009
- ...that measure the interactions of [[photon]]s, in the visible, infrared or ultraviolet spectra, with elements being analyzed, as the materials under test variousl361 bytes (51 words) - 16:03, 18 May 2010
- {{dambigbox|the Wisconsin Ultraviolet Photo-Polarimeter Experiment|Wisconsin}} ...onsin Ultraviolet Photo-Polarimeter Experiment''' WUPPE was one of three [[ultraviolet]] [[telescope|telescopes]] on the [[ASTRO-1 mission]] flown on the [[space3 KB (427 words) - 13:04, 9 August 2023
- ...sorb, or reflect electromagnetic energy in the infrared, visible light, or ultraviolet spectra, where the value is knowledge of the type of energy detected434 bytes (59 words) - 18:43, 12 September 2009
- {{r|International Ultraviolet Explorer}} {{r|Ultraviolet}}2 KB (294 words) - 14:14, 6 April 2024
- {{r|Ultraviolet}}299 bytes (37 words) - 17:08, 22 March 2024
- {{r|Ultraviolet}}465 bytes (58 words) - 15:41, 11 January 2010
- ...tion concerned with understanding light, — typically in the visible, ultraviolet, and infrared ranges of the electromagnetic spectrum — and harnessing718 bytes (101 words) - 11:27, 7 April 2010
- {{r|Ultraviolet}}442 bytes (57 words) - 19:14, 11 January 2010
- {{r|Ultraviolet}}454 bytes (58 words) - 16:44, 11 January 2010
- {{r|Ultraviolet}}510 bytes (65 words) - 11:35, 31 December 2022
- {{r|Ultraviolet}}578 bytes (75 words) - 19:52, 11 January 2010
- {{r|Ultraviolet}}626 bytes (81 words) - 18:35, 11 January 2010
- {{r|International Ultraviolet Explorer}}707 bytes (90 words) - 19:56, 11 January 2010
- ...cule]]s, as well as electromagnetic fields at frequencies primarily in the ultraviolet to microwave range. Included are the interactions of these fields with atom597 bytes (94 words) - 21:36, 9 October 2020
- The '''Galaxy Evolution Explorer''' is an [[orbit|orbiting]] [[ultraviolet]] [[space telescope]] that was launched on [[April 28]], 2003. A [[Pegasus During its nominal 29 month mission is making observations at [[ultraviolet]] wavelengths to measure the history of star formation in the [[Universe]]2 KB (315 words) - 13:38, 26 September 2007
- {{r|International Ultraviolet Explorer}}936 bytes (115 words) - 12:57, 15 March 2024
- {{r|Ultraviolet}}936 bytes (120 words) - 19:37, 11 January 2010
- {{r|Ultraviolet}}831 bytes (112 words) - 19:43, 11 January 2010
- ...e oxygen [[atom]]s. It is produced in the Earth's [[stratosphere]] when [[ultraviolet radiation]] causes diatomic oxygen (O<sub>2</sub>) to dissociate into two s878 bytes (122 words) - 22:17, 16 April 2009
- The sun's [[ultraviolet ray]]s consists of UVA and UVB.<ref name="pmid18772844">{{cite journal |aut900 bytes (128 words) - 20:21, 8 September 2008
- {{r|Ultraviolet absorption spectometry}}1 KB (102 words) - 17:36, 9 June 2010
- {{r|Ultraviolet}}1 KB (145 words) - 12:05, 6 March 2024
- ...an astronomical [[observatory]] [[satellite]] primarily designed to take [[ultraviolet]] [[Electromagnetic spectrum|spectra]]. The satellite was a collaborative p <caption><br>'''International Ultraviolet Explorer (IUE)'''</caption>7 KB (1,076 words) - 09:16, 6 March 2024
- ...s, or, as with the [[FIM-92 Stinger]], for a combination of infrared and [[ultraviolet]] energy. While the first such flares burned [[magnesium]], most modern sen1 KB (169 words) - 10:44, 8 April 2024
- {{r|International Ultraviolet Explorer}}1 KB (178 words) - 13:07, 10 January 2021
- ...e that does not ionize biological molecules — from the higher-energy ultraviolet, through the intermediate-energy visible, to the lower-energy infrared rang * Solar Ultraviolet Protection Provided by Human Head Hair4 KB (478 words) - 15:45, 3 August 2012
- ** Far Ultraviolet Spectroscopic Explorer|FUSE ** Extreme Ultraviolet Explorer6 KB (725 words) - 12:06, 9 March 2021
- {{r|International Ultraviolet Explorer}}1 KB (180 words) - 11:54, 31 December 2022
- ...ed a series of high resolution far- (900-1560 Å) and near- (1650-3150 Å) [[ultraviolet]] spectral scans of 551 objects, primarily bright [[stars]], from 1972 to 1 ...t, inclined at 35 degrees, on 21 August 1972. The main experiment was an [[ultraviolet telescope]]. However, it also contained a cosmic X-ray experiment provided3 KB (435 words) - 07:27, 26 September 2007
- {{r|Ultraviolet}}2 KB (216 words) - 06:40, 23 March 2022