Neutrino Oscillation: The phenomenon where neutrinos can change their flavor (electron, muon, or tau neutrino) as they travel through space, which was used to explain the solar neutrino problem.
Solar Neutrino Problem: The discrepancy between the number of solar neutrinos detected on Earth and the number predicted by the Standard Solar Model, which was resolved by the discovery of neutrino oscillation.
Standard Solar Model: A theoretical model that describes the internal structure and energy-generating processes of the Sun, including the production of solar neutrinos.