RICH detectors use this effect to measure the velocity of subatomic particles. In a periodic medium, such as the surface of a diffraction grating, this effect requires no minimum velocity. Its spectral intensity is approximately proportional to the frequency, according to the (*) Frank-Tamm formula, so most of its energy is actually in the UV. Observatories such as IceCube and Super-Kamiokande use this effect to detect neutrinos. Created when a particle travels through a medium faster than the local speed of light, for ten points name of this type of radiation characte
RICH detectors use this effect to measure the velocity of subatomic particles. In a periodic medium, such as the surface of a diffraction grating, this effect requires no minimum velocity. Its spectral intensity is approximately proportional to the frequency, according to the (*) Frank-Tamm formula, so most of its energy is actually in the UV. Observatories such as IceCube and Super-Kamiokande use this effect to detect neutrinos. Created when a particle travels through a medium faster than the local speed of light, for ten points name of this type of radiation characterized by a blue glow in nuclear reactors.
RICH detectors use this effect to measure the velocity of subatomic particles.
{Cherenkov} radiation