145 citations · 369 across the 6 of their papers we have counts for
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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…
High Frequency Waves in Chromospheric Spicules
W. Bate, D. B. Jess, V. M. Nakariakov +6
Using high cadence observations from the Hydrogen-alpha Rapid Dynamics camera imaging system on the Dunn Solar Telescope, we present an investigation of the statistical properties…
Kink oscillations of coronal loops
V. M. Nakariakov, S. A. Anfinogentov, P. Antolin +13
Kink oscillations of coronal loops, i.e., standing kink waves, is one of the most studied dynamic phenomena in the solar corona. The oscillations are excited by impulsive energy re…
Seismological constraints on the solar coronal heating function
D. Y. Kolotkov, T. J. Duckenfield, V. M. Nakariakov
The hot solar corona exists because of the balance between radiative and conductive cooling and some counteracting heating mechanism which remains one of the major puzzles in solar…
Excitation of decay-less transverse oscillations of coronal loops by random motions
A. N. Afanasyev, T. Van Doorsselaere, V. M. Nakariakov
The relatively large-amplitude decaying regime of transverse oscillations of coronal loops has been known for two decades and interpreted in terms of MHD kink modes of cylindrical…
Damping of slow magnetoacoustic oscillations by the misbalance between heating and cooling processes in the solar corona
D. Y. Kolotkov, V. M. Nakariakov, D. I. Zavershinskii
Rapidly decaying slow magnetoacoustic waves are regularly observed in the solar coronal structures, offering a promising tool for a seismological diagnostics of the coronal plasma,…