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- CLIO abstract "CLIO is the Cryogenic Laser Interferometer Observatory, a prototype detector for gravitational waves. It is testing cryogenic mirror technologies for the future Large Cryogenic Gravity Telescope (LCGT).It is an optical interferometer with two perpendicular arms 100 m long. Uniquely, the mirrors are cooled to 20 K. This reduces various thermal noise sources which trouble other gravity observatories, but cooling the mirrors (which is heated by the powerful laser used in the interferometer) while keeping them isolated from vibrations is difficult.CLIO is situated 1000 m underground in the Kamioka mine, Gifu Prefecture, Japan.CLIO is one of the science facilities for physics of the Institute for Cosmic Ray Research of the University of Tokyo.".
- CLIO wikiPageID "19114702".
- CLIO wikiPageRevisionID "593701797".
- CLIO hasPhotoCollection CLIO.
- CLIO subject Category:Effects_of_gravitation.
- CLIO subject Category:General_relativity.
- CLIO subject Category:Gravitation.
- CLIO type Consequence111410625.
- CLIO type EffectsOfGravitation.
- CLIO type Phenomenon100034213.
- CLIO type PhysicalEntity100001930.
- CLIO type Process100029677.
- CLIO comment "CLIO is the Cryogenic Laser Interferometer Observatory, a prototype detector for gravitational waves. It is testing cryogenic mirror technologies for the future Large Cryogenic Gravity Telescope (LCGT).It is an optical interferometer with two perpendicular arms 100 m long. Uniquely, the mirrors are cooled to 20 K.".
- CLIO label "CLIO".
- CLIO label "CLIO".
- CLIO label "低温レーザー干渉計重力波観測装置".
- CLIO sameAs CLIO.
- CLIO sameAs 低温レーザー干渉計重力波観測装置.
- CLIO sameAs m.04j9pl7.
- CLIO sameAs Q3648786.
- CLIO sameAs Q3648786.
- CLIO sameAs CLIO.
- CLIO wasDerivedFrom CLIO?oldid=593701797.
- CLIO isPrimaryTopicOf CLIO.