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Conclusions In summary, the results of global, local helioseismology as well as 3D radiative hydrodynamic simulations show that the NSSL (Near Sub Surface La yer) occupying the top 15% of the solar convection zone, the depth range ≈ 30 − · 1998 · DOI 10.48550/arxiv.astro-ph/970

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Improving Our Knowledge of the Solar Near-Surface Shear Layer: The Special Case of the Leptocline

astro-ph.SR · 2025-01-14 · conditional · novelty 4.0

The Sun's near-surface shear layer contains a distinct 8 Mm deep leptocline with strong rotational gradients, enhanced turbulence, and cycle-dependent variations.

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Improving Our Knowledge of the Solar Near-Surface Shear Layer: The Special Case of the Leptocline astro-ph.SR · 2025-01-14 · conditional · none · ref 6
The Sun's near-surface shear layer contains a distinct 8 Mm deep leptocline with strong rotational gradients, enhanced turbulence, and cycle-dependent variations.

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