Abstract The coronal heating problem — one of the longest-standing puzzles in solar physics — asks why the corona reaches temperatures of 1–3 million K while the photosphere is only ~5800 K. Classical mechanisms (wave heating, magnetic reconnection) explain only part of the required energy. Global Complexity–Stability Theory (GCST) offers a novel interpretation: the corona is the external dissipation layer for accumulated structural debt in the Sun’s magnetic field. In the interior and chromosphere, the rate of complexity generation α significantly exceeds local dissipation γ, forcing structural debt D to be transported upward. In the corona, where γ is minimal, this debt is forcibly released through plasma heating — the mechanism behind the million-degree temperatures. The core GCST stability condition is In the photosphere/chromosphere G_⊙ ≈ 0. 7–0. 9 (debt accumulation) ; in the corona G_⊙ << 0. 1 → rapid debt release → coronal heating.
Roman Lukin (Thu,) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: