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Cited article:

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VELOCITY-SHEAR-INDUCED MODE COUPLING IN THE SOLAR ATMOSPHERE AND SOLAR WIND: IMPLICATIONS FOR PLASMA HEATING AND MHD TURBULENCE

Joseph V. Hollweg, Edisher Kh. Kaghashvili and Benjamin D. G. Chandran
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https://doi.org/10.1088/0004-637X/769/2/142

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Multi-scale Physics in Coronal Heating and Solar Wind Acceleration

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Space Sciences Series of ISSI, Multi-scale Physics in Coronal Heating and Solar Wind Acceleration 38 397 (2011)
https://doi.org/10.1007/978-1-4614-6461-7_26

Self-heating and its possible relationship to chromospheric heating in slowly rotating stars

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Monthly Notices of the Royal Astronomical Society (2010)
https://doi.org/10.1111/j.1365-2966.2009.16159.x

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Overreflection and Generation of Gravito‐Alfven Waves in Solar‐Type Stars

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The Astrophysical Journal 664 (2) 1221 (2007)
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Transient shear instability of differentially rotating and self-gravitating dusty plasma

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Swirling astrophysical flows – efficient amplifiers of Alfvén waves!?

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Astronomy & Astrophysics 399 (2) 421 (2003)
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