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Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves

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ELECTRIC CURRENT FILAMENTATION AT A NON-POTENTIAL MAGNETIC NULL-POINT DUE TO PRESSURE PERTURBATION

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Multi-mode quasi-periodic pulsations in a solar flare

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2D MHD AND 1D HD MODELS OF A SOLAR FLARE—A COMPREHENSIVE COMPARISON OF THE RESULTS

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IMAGING OBSERVATION OF QUASI-PERIODIC DISTURBANCES' AMPLITUDES INCREASING WITH HEIGHT IN THE POLAR REGION OF THE SOLAR CORONA

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FREQUENCY-DEPENDENT DAMPING IN PROPAGATING SLOW MAGNETO-ACOUSTIC WAVES

S. Krishna Prasad, D. Banerjee and T. Van Doorsselaere
The Astrophysical Journal 789 (2) 118 (2014)
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Effect of partial ionization on wave propagation in solar magnetic flux tubes

R. Soler, A. J. Díaz, J. L. Ballester and M. Goossens
Astronomy & Astrophysics 551 A86 (2013)
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Fast damping of acoustic waves in solar coronal loops as a result of their radiation

D. B. Bembitov, I. S. Veselovsky and B. B. Mikhalyaev
Geomagnetism and Aeronomy 53 (8) 1013 (2013)
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Magnetohydrodynamic waves and coronal seismology: an overview of recent results

Ineke De Moortel and Valery M. Nakariakov
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 370 (1970) 3193 (2012)
https://doi.org/10.1098/rsta.2011.0640