Neutrino observatories

is a neutrino observatory located under Mount Ikeno near the city of Hida, Gifu Prefecture, Japan. It is operated by the Institute for Cosmic Ray Research, University of Tokyo with the help of an international team. It is located 1,000 m (3,300 ft) underground in the Mozumi Mine in Hida's Kamioka area. The observatory was designed to detect high-energy neutrinos, to search for proton decay, study solar and atmospheric neutrinos, and keep watch for supernovae in the Milky Way galaxy.

neutrino observatory constructed under the ice at the South Pole

thumb|The KM3NeT LOM (Launching vehicle of Optical Modules) being loaded onto the RV Pelagia deployment vessel. A full string detection is rolled onto the LOM. After arrival at the seabed the string is unrolled to its full length.|250x250pxthumb|KM3NeT Digital Optical Module (DOM) in the laboratory|250x250pxThe Cubic Kilometre Neutrino Telescope, or KM3NeT, is a European research infrastructure located on the bed of the Mediterranean Sea at depths of over 2 kilometres. It hosts water Cherenkov neutrino telescopes designed to detect and study neutrinos from distant astrophysical sources as well

physics apparatus which is designed to study neutrinos

underground laboratory in Ontario, Canada

thumb|318px|Overview of the Hyper-Kamiokande experiment

physics laboratory in Assergi, Italy

neutrino detector in the Mediterranean Sea

Borexino is a deep underground particle physics experiment to study low energy (sub-MeV) solar neutrinos. The detector is the world's most radio-pure liquid scintillator calorimeter and is protected by 3,800 meters of water-equivalent depth (a volume of overhead rock equivalent in shielding power to that depth of water). The scintillator is pseudocumene and PPO which is held in place by a thin nylon sphere. It is placed within a stainless steel sphere which holds the photomultiplier tubes (PMTs) used as signal detectors and is shielded by a water tank to protect it against external radiation.

neutrino experiment in Jiangmen, China

neutrino telescope located beneath the Amundsen–Scott South Pole Station

underground experiment to count Solar neutrinos

scientific laboratory mainly studying neutrinos; located in the Caucasus mountains in Russia

underground neutrino and gravitational wave observatory in Kamioka, Japan

GALLEX or Gallium Experiment was a radiochemical neutrino detection experiment that ran between 1991 and 1997 at the Laboratori Nazionali del Gran Sasso (LNGS). This project was performed by an international collaboration of French, German, Italian, Israeli, Polish and American scientists led by the Max-Planck-Institut für Kernphysik Heidelberg. After brief interruption, the experiment was continued under a new name GNO (Gallium Neutrino Observatory) from May 1998 to April 2003.

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Indian physics research project

neutrino oscillation experiment in Japan