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Cited article:

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An Iterative OLA Method for Inversion of Solar Spectropolarimetric Data. I. Single- and Multiple-variable Inversions of Thermodynamic Quantities

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High-frequency Wave Power Observed in the Solar Chromosphere with IBIS and ALMA

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Slow magneto-acoustic waves in simulations of a solar plage region carry enough energy to heat the chromosphere

N. Yadav, R. H. Cameron and S. K. Solanki
Astronomy & Astrophysics 652 A43 (2021)
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Dynamics of small-scale magnetic fields on the Sun: observations and numerical simulations

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Evidence of Shock-driven Turbulence in the Solar Chromosphere

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Self‐consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence

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Determination of the Acoustic Wave Flux in the Lower Solar Chromosphere

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Response Functions of the Ultraviolet Filters ofTRACEand the Detectability of High‐Frequency Acoustic Waves

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On the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant Heliosphere

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On the Validity of Acoustically Heated Chromosphere Models

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Numerical simulation of the three-dimensional structure and dynamics of the non-magnetic solar chromosphere

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On the Origin of the Basal Emission from Stellar Atmospheres: Analysis of Solar CiiLines

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