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Leenaarts, J · 2007

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astro-ph.SR 1

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2026 1

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UNVERDICTED 1

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Chromospheric dynamics and the O I 135.6~nm spectral line

astro-ph.SR · 2026-05-04 · unverdicted · novelty 4.0

Simulations identify photospheric magnetic field strength as the main driver of Mg II core line widths in quiet Sun regions, with non-equilibrium hydrogen ionization and 3D radiative transfer key in active regions.

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  • Chromospheric dynamics and the O I 135.6~nm spectral line astro-ph.SR · 2026-05-04 · unverdicted · none · ref 9

    Simulations identify photospheric magnetic field strength as the main driver of Mg II core line widths in quiet Sun regions, with non-equilibrium hydrogen ionization and 3D radiative transfer key in active regions.