Ultraviolet radiation is detected by photographic plates and by means of the photoelectric effect
in photomultiplier tubes.
Not exact matches
All of that,
in turn, is surrounded by 1,879
photomultiplier tubes, which pick up flashes of light produced as antineutrinos collide with protons
in the liquid - filled balloon.
The wispy particles can not be observed directly, however, so the 39 - meter - diameter, 41 - meter - high observation tank is filled with water and lined with
photomultiplier tubes that can catch a distinctive glow, known as Cerenkov radiation, produced when neutrinos smash into atomic particles
in the water.
Photomultiplier tubes within the detector, shown above, detect light produced
in interactions possibly caused by dark matter particles.
When a low - energy neutrino or antineutrino from a supernova collides with a water molecule
in the tank, the resulting light signal is recorded by about 100 of 13,000
photomultipliers, ultrasensitive light - detecting devices that turn a tiny flash of light into a larger recordable burst of electricity.
Besides the advantage of needing far fewer
photomultiplier tubes to detect high - energy neutrinos, Domogatsky pointed out that only a detector
in the Northern Hemisphere could see neutrinos from the center of our galaxy.