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The centroid speed as a characteristic of the group speed of solar coronal fast magnetoacoustic wave trains
Dmitrii Y. Kolotkov, Valery M. Nakariakov, Maximilien Cloesen
The highly-filamented nature of the coronal plasma significantly influences dynamic processes in the corona such as magnetohydrodynamic waves and oscillations. Fast magnetoacoustic…
Polarisation of decayless kink oscillations of solar coronal loops
Sihui Zhong, Valery M. Nakariakov, Dmitrii Y. Kolotkov +4
Decayless kink oscillations of plasma loops in the solar corona may contain an answer to the enigmatic problem of solar and stellar coronal heating. The polarisation of the oscilla…
Bayesian evidence for two slow-wave damping models in hot coronal loops
I. Arregui, D. Y. Kolotkov, V. M. Nakariakov
We compute the evidence in favour of two models, one based on field-aligned thermal conduction alone and another that includes thermal misbalance as well, in explaining the damping…
Quasi-periodic pulsations in solar flares: a key diagnostic of energy release on the Sun
Andrew Inglis, Laura Hayes, Silvina Guidoni +18
Solar flares are among the most powerful and disruptive events in our solar system, however the physical mechanisms driving and transporting this energetic release are not fully un…
Stability of slow magnetoacoustic and entropy waves in the solar coronal plasma with thermal misbalance
Dmitrii Y. Kolotkov, Valery M. Nakariakov, Joseph B. Fihosy
The back-reaction of the perturbed thermal equilibrium in the solar corona on compressive perturbations, also known as the effect of wave-induced thermal misbalance, is known to re…