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The 23 pages that link to Photomultiplier tube, each with the reason it gives.

• Fluorescence microscopyRelated: It can measure the weak emitted light collected in fluorescence imaging.

• Particle detectorRelated: It amplifies the weak scintillation light generated by many detector materials.

• Super-KamiokandeRelated: Thousands of these sensors line the tank and register faint Cherenkov light.

• IceCube Neutrino ObservatoryRelated: These sensors register faint Cherenkov flashes in the Antarctic ice.

• Confocal microscopyRelated: It commonly measures the weak fluorescence collected from each scanned point.

• Optically stimulated luminescenceRelated: It detects the faint luminescence emitted from stimulated mineral grains.

• Sudbury Neutrino ObservatoryRelated: Thousands of photomultiplier tubes registered faint flashes inside SNO’s water shield.

• KamiokandeRelated: Photomultiplier tubes lining Kamiokande’s tank registered faint Cherenkov flashes.

• Scintillation detectorRelated: Photomultiplier readout enabled scintillation counters to detect flashes electronically.

• Cherenkov detectorRelated: Photomultipliers detect the faint photons collected from the radiator.

• Masatoshi KoshibaRelated: These sensors recorded the faint flashes produced in Koshiba’s water detectors.

• Sodium iodideRelated: It detects the light flashes produced when radiation excites a NaI crystal.

• Atomic emission spectroscopyRelated: It can measure weak emission lines after the spectrometer isolates them.

• ScintillatorRelated: It detects and amplifies the weak flashes produced by many scintillators.

• BiophotonRelated: Experiments use photon-counting detectors to measure emissions too faint for unaided vision.