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Cited article:

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Fast-to-Alfvén Mode Conversion and Ambipolar Heating in Structured Media. II. Numerical Simulation

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The Astrophysical Journal 883 (2) 179 (2019)
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First Ten Years of Hinode Solar On-Orbit Observatory

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Propagation of Torsional Alfvén Waves from the Photosphere to the Corona: Reflection, Transmission, and Heating in Expanding Flux Tubes

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THE SOLAR CHROMOSPHERE OBSERVED AT 1 Hz AND 0.″2 RESOLUTION

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ACCELERATION OF TYPE 2 SPICULES IN THE SOLAR CHROMOSPHERE. II. VISCOUS BRAKING AND UPPER BOUNDS ON CORONAL ENERGY INPUT

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Ionized Plasma and Neutral Gas Coupling in the Sun’s Chromosphere and Earth’s Ionosphere/Thermosphere

J. E. Leake, C. R. DeVore, J. P. Thayer, et al.
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Magnetic-diffusion-driven shear instability of solar flux tubes

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CONDITIONS FOR PHOTOSPHERICALLY DRIVEN ALFVÉNIC OSCILLATIONS TO HEAT THE SOLAR CHROMOSPHERE BY PEDERSEN CURRENT DISSIPATION

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The Astrophysical Journal 735 (1) 45 (2011)
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SIMULATION OF MAGNETOHYDRODYNAMIC SHOCK WAVE GENERATION, PROPAGATION, AND HEATING IN THE PHOTOSPHERE AND CHROMOSPHERE USING A COMPLETE ELECTRICAL CONDUCTIVITY TENSOR

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Evidence for a Current Sheet above a Sunspot Umbra

A. Tritschler, H. Uitenbroek and K. Reardon
The Astrophysical Journal 686 (1) L45 (2008)
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Magnetohydrodynamic Simulations of Solar Chromospheric Dynamics Using a Complete Electrical Conductivity Tensor

Farzad Kazeminezhad and Michael L. Goodman
The Astrophysical Journal Supplement Series 166 (2) 613 (2006)
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Collisional dissipation of Alfvén waves in a partially ionised solar chromosphere

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Astronomy & Astrophysics 442 (3) 1091 (2005)
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Self‐consistent Magnetohydrodynamic Modeling of Current Sheet Structure and Heating Using Realistic Descriptions of Transport Processes

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The Astrophysical Journal 632 (2) 1168 (2005)
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