KnowraSudbury Neutrino ObservatoryLinked fromLinked fromThe 12 pages that link to Sudbury Neutrino Observatory, each with the reason it gives.All 12Broader topic 5Related 6Compared with 1NeutrinoBroader topic: Its results showed that missing solar electron neutrinos had changed flavor.Neutrino oscillationRelated: Its neutral-current measurement showed solar electron neutrinos changed into other active flavors.Neutrino massRelated: It showed that missing electron neutrinos had changed flavor, confirming oscillation as the solar solution.Solar neutrino problemBroader topic: Its neutral-current measurement counted all active flavors and demonstrated that the missing electron neutrinos had changed flavor.Proton decayRelated: Its heavy-water searches provided independent constraints on proton decay.Solar neutrinoBroader topic: Its flavor-sensitive measurements showed that the missing electron neutrinos had changed flavor.KamiokandeCompared with: Its flavor-sensitive measurements resolved the solar neutrino problem beyond Kamiokande’s capabilities.Raymond Davis Jr.Related: It later showed that neutrinos changed flavor, resolving the deficit in Davis's measurements.Homestake experimentRelated: Its measurements resolved the deficit by counting all active neutrino flavors.Electron neutrinoBroader topic: It separated electron-neutrino flux from the total active solar-neutrino flux.Arthur B. McDonaldBroader topic: Its flavor-sensitive reactions let McDonald’s team compare total neutrinos with electron neutrinos.Takaaki KajitaRelated: Its measurements independently confirmed flavor transformation, complementing Kajita’s atmospheric evidence.