enow.com Web Search

Search results

1. Results from the WOW.Com Content Network

2. KM3NeT - Wikipedia

   en.wikipedia.org/wiki/KM3NeT

   Arrays of thousands of optical sensor modules detect the faint Cherenkov light in the deep sea from charged particles originating from collisions of the neutrinos and the water or rock in the vicinity of the detector. The position and direction of the optical modules and the time of arrival of the light on the photomultipliers inside is ...

3. Ocean optics - Wikipedia

   en.wikipedia.org/wiki/Ocean_optics

   A scientist measures K d (PAR) from a boat in the Chesapeake Bay. This is a measure of downwelling light attenuation using a flat-topped light sensor (small brown metal cylinder at left), called a cosine collector, to measure the light coming down onto a flat surface from above.

4. ANTARES (telescope) - Wikipedia

   en.wikipedia.org/wiki/ANTARES_(telescope)

   In addition to the main optical detector for cosmic neutrinos, the ANTARES experiment also houses a number of instruments for the study of the deep sea environment, such as salinity and oxygen probes, sea current profilers and instrumentation for the measurement of light transmission and sound velocity.

5. AOL

   search.aol.com

   The search engine that helps you find exactly what you're looking for. Find the most relevant information, video, images, and answers from all across the Web.

6. Neutrino detector - Wikipedia

   en.wikipedia.org/wiki/Neutrino_detector

   Consisting of an array of twelve separate 350 meter-long vertical detector strings 70 meters apart, each with 75 photomultiplier optical modules, this detector uses the surrounding sea water as the detector medium. The next generation deep sea neutrino telescope KM3NeT will have a total instrumented volume of about 5 km 3. The detector will be ...

7. List of neutrino experiments - Wikipedia

   en.wikipedia.org/wiki/List_of_neutrino_experiments

   Kamioka Liquid Scintillator Antineutrino Detector R ν e: ν e + p → e + + n: CC LOS: Scintillation: 1.8 MeV Kamioka, Japan 2002– KM3NeT: KM3 Neutrino Telescope S, ATM, CR, SN, AGN, PUL ν μ, ν e, ν τ: Sea water (≈5 km 3) Cherenkov Mediterranean Sea: 2014– LAGUNA: Large Apparatus studying Grand Unification and Neutrino Astrophysics ...