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  • ...that measure the interactions of [[photon]]s, in the visible, infrared or ultraviolet spectra, with elements being analyzed, as the materials under test variousl
    361 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 [[space
    3 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 detected
    434 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 harnessing
    718 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 atom
    597 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 s
    878 bytes (122 words) - 22:17, 16 April 2009
  • The sun's [[ultraviolet ray]]s consists of UVA and UVB.<ref name="pmid18772844">{{cite journal |aut
    900 bytes (128 words) - 20:21, 8 September 2008
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