Heliopause Thermal Anomaly under the DQ-12 Framework

Contemporary astrophysics faces two major thermal anomalies at the limits of stellar influence: the problem of solar corona heating (where temperatures rise from 5,500 °C at the surface to over 1,000,000 °C in the atmosphere) and the 50,000 °C "plasma wall" detected by the Voyager probes at the heliopause . The Standard Model attempts to explain these phenomena in isolation by resorting to complex models of magnetic reconnection and shock waves. In this work, we apply the Quantum Diffusion Framework (DQ-12) to unify both phenomena under a single continuum mechanics. By modeling the stellar system as a macroscopic vortex within a topological space fluid, we demonstrate that both thermal anomalies are a direct result of thermodynamic dissipation due to phase friction (shear). The corona and the heliopause represent the inner and outer boundary layers of the vortex, respectively, where the geometric stress of the medium generates a sharp increase in temperature.