Submitted:
08 September 2025
Posted:
09 September 2025
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Abstract
Keywords:
Introduction
- Insufficient Energy Supply: Known mechanisms account for only 10-20% of required heating energy.
- Spatial Distribution Mismatch: Predictions contradict SDO/AIA thermal maps in quiet coronal regions.
- Energy Scale Gap: No bridge between quantum-scale physics and macroscopic phenomena.
Methodological Introduction
- Theoretical Foundation: Energy Transfer via -Gradients
- SDO/AIA EUV imaging (0.5 acres resolution) in Fe XVIII (94 Å), Fe XXIV (193 Å), and Fe XIV (211 Å) lines for <15% error temperature mapping.
- NuSTAR hard X-ray spectroscopy (2-30 keV) detecting >five MK active regions.
- SDO/HMI vector magneto grams (10 Gauss precision, 45s cadence).
- DKIST/ViSP non-thermal velocity measurements (380-860 nm spectral coverage).
- ALMA Band 6 radio observations (1.3 mm, 0.1 THz spectral resolution).
- -fluctuations during flares:Detectable by Solar Orbiter/EUI (0.5s temporal resolution).
- Terahertz emission from active regions:Observable with ALMA Band 10.
- Spatial -T correlation:
Discussion and Conclusion
| Model | Accuracy (%) | Free Parameters | Multi-Spectral Consistency (χ²/ν) |
| CEIT | 98.7 ± 0.5 | 3 | 0.95 |
| Nano flares | 92.1 ± 1.2 | 6 | 2.3 |
| Alfven Waves | 88.5 ± 2.0 | 4 | 3.1 |
| Turbulent Heating | 85.3 ± 3.1 | 5 | 4.7 |
- Magnetic-topology invariance: Heating efficiency persists in both open/closed field regions.
- Observed non-thermal broadening: Directly linked to -ffluctuations via .
- Rapid temperature scaling: accounts for impulsive heating in flares.
| Prediction | Detection Method | Instrument | Timeline |
| during flares | EUV spectroscopy | Solar Orbiter/EUI | 2026 |
| Terahertz emission () | Sub-mm interferometry | ALMA (Band 10) | 2027 |
| Spatial – correlation () | High-resolution imaging | DKIST/HiC | 2028 |
Concluding Remarks
- Eliminates ad hoc assumptions by deriving heating from first principles.
- Unifies solar/stellar coronae physics under a single scaling law ().
- Provides falsifiable predictions for next-generation observatories (DKIST, HUBS, Athena).
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