Major types of neutrino detectors are classified by the detection medium and interaction technique:
Detector type, Detection medium, Main signal, Example experiments
Water Cherenkov Detector: Pure water, Cherenkov light from charged particles, Super-Kamiokande, Hyper-Kamiokande
Heavy-water Cherenkov Detector: D₂O, Cherenkov light + neutral-current sensitivity, SNO
Ice Cherenkov Detector: Antarctic/glacial ice, Cherenkov light, IceCube, PINGU concept
Deep-Sea / Lake Cherenkov Detector: Seawater or lake water, Cherenkov light, KM3NeT, Baikal-GVD, ANTARES
Liquid Scintillator Detector: Organic scintillator, Scintillation light, KamLAND, Borexino, JUNO
Liquid Argon Time Projection Chamber: Liquid argon, Ionization charge + scintillation light, DUNE, ICARUS, MicroBooNE
Tracking Calorimeter Detector: Iron/scintillator, plastic, emulsion, etc., Particle tracks + energy deposition, MINOS, NOvA, OPERA
Nuclear Emulsion Detector: Photographic emulsion layers, Microscopic charged-particle tracks, OPERA, DONUT
Radiochemical Detector: Chlorine or gallium, Neutrino-induced nuclear transmutation, Homestake, GALLEX, SAGE
Coherent elastic neutrino–nucleus scattering detector: CsI, Ge, Ar, Xe, etc., Tiny nuclear recoil, COHERENT
Radio Neutrino Detector: Ice, salt, lunar regolith, Askaryan radio pulse, ARA, ARIANNA, RNO-G
Acoustic Neutrino Detector: Water or ice, Pressure pulse from particle shower, Experimental /R&D concepts
Cherenkov Telescope Array Observatory (CTAO): Air Shower.
Simple Terms:
Low-energy solar / reactor neutrinos → Scintillator, radiochemical, water Cherenkov
Accelerator neutrinos → Liquid argon TPC, tracking calorimeter, Cherenkov
High-energy cosmic neutrinos → ice / water Cherenkov, radio detectors
Ultra-high-energy neutrinos → Radio and acoustic detection concepts