Solar Magnetic Loops as Coherence Tension Architectures: A MID/QC Interpretation of Coronal Structure and Eruption

Solar magnetic loops are traditionally modeled as plasma structures shaped by magnetic field lines and pressure balance, yet their stability, discreteness, helicity, and explosive reconnection remain only partially understood. In the MID/QC framework, these loops are reinterpreted as coherence‑tension architectures carved into the substrate by polarized submergent quanta within the Sun’s deep coherence well. Loops trace coherence channels and torsion structures in the substrate rather than abstract magnetic field lines in plasma. This perspective provides mechanistic explanations for loop stability, quantized bundling, helicity buildup, and rapid reconnection. Thermal conditions near the Sun modulate substrate behavior, with temperature‑dependent coherence and tension properties influencing loop dynamics. Observational strategies comparing sun‑adjacent regions to mid‑space baselines may allow indirect inference of substrate tension from coronal and heliospheric behavior.