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Rev. Lett."],"accepted":{"date-parts":[[2026,7,14]]},"abstract":"<jats:p>\n                    Matter-induced neutrino flavor mixing (the Mikheyev-Smirnov-Wolfenstein, or MSW, effect) is a central prediction of the neutrino mixing framework, but it has not been conclusively observed. Direct observation of the energy-dependent MSW transition in the solar electron-neutrino survival probability would solve this, but backgrounds have been prohibitive. We show that our new technique for suppressing muon-induced spallation backgrounds will allow JUNO to measure the MSW transition at\n                    <a:math xmlns:a=\"http:\/\/www.w3.org\/1998\/Math\/MathML\" display=\"inline\">\n                      <a:mo>&gt;<\/a:mo>\n                      <a:mrow>\n                        <a:mn>4<\/a:mn>\n                        <a:mi>\u03c3<\/a:mi>\n                      <\/a:mrow>\n                    <\/a:math>\n                    significance in 10\u00a0years. 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