Standard solar physics attributes flares to magnetic reconnection—twisted field lines releasing stored energy. This framework describes the electromagnetic signature but fails to explain the underlying mechanical cause. This study proposes that solar flares are contamination purge events: the periodic expulsion of fusion byproducts (primarily helium) that accumulate near the stellar core and migrate outward until surface breach. Flare frequency and intensity become diagnostic indicators of stellar health—a star that flares regularly is successfully selfmaintaining; a star that stops flaring has lost the purge war and is accumulating toward eventual phase collapse. Analysis of flare behavior across metallicity ranges supports this framework: metal-poor stars exhibit violent, stochastic flaring (minimal contamination architecture), while metal-rich stars show regular, lower-energy cycles (organized contamination layers enabling rhythmic purging).
Matt Webb (Wed,) studied this question.