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.