Linked from

The 11 pages that link to Kamiokande, each with the reason it gives.

• Particle detectorBroader topic: Its supernova-neutrino measurements provided direct evidence from the 1987 stellar explosion.

• Solar neutrino problemBroader topic: It independently confirmed the deficit and showed that detected neutrinos came from the Sun.

• Super-KamiokandeBroader topic: Its results and design informed the larger Super-Kamiokande successor.

• SN 1987ABroader topic: Kamiokande detected neutrinos from SN 1987A before the optical discovery.

• Solar neutrinoBroader topic: It confirmed the deficit with directional, real-time measurements.

• Sudbury Neutrino ObservatoryRelated: Its observations provided an earlier, different approach to measuring neutrinos from the Sun.

• Raymond Davis Jr.Related: Its independent observations helped confirm the solar-neutrino deficit found by Davis.

• Homestake experimentRelated: Its independent solar-neutrino measurements confirmed a deficit relative to expectations.

• Masatoshi KoshibaBroader topic: Koshiba led the experiment that first detected neutrinos from a supernova.

• Arthur B. McDonaldRelated: Its solar-neutrino measurements strengthened evidence for a deficit before Sudbury resolved its cause.

• Takaaki KajitaBroader topic: Kajita’s early work there identified an atmospheric-neutrino discrepancy.