Measurement of Turbulence Injection Scale Down to the Chromosphere
The solar atmosphere displays a sharp temperature gradient, starting from spicules in the chromosphere at 2 × 10 ^4 K, outward into the corona exceeding ${10}^{6}$ K. Plasma turbulence produced by the transverse motion of magnetic fields anchored in the photosphere is likely the energy source produc...
שמור ב:
| Principais autores: | , , , |
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| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
IOP Publishing
2025-01-01
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| סדרה: | The Astrophysical Journal Letters |
| נושאים: | |
| גישה מקוונת: | https://doi.org/10.3847/2041-8213/ada363 |
| תגים: |
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