A new look at the frequency-dependent damping of slow-mode waves in the solar corona
Dmitrii Y. Kolotkov, Valery M. Nakariakov

TL;DR
This paper investigates the frequency-dependent damping of slow magnetoacoustic waves in the solar corona, revealing how thermal misbalance influences wave damping and matches observational data.
Contribution
It introduces a modified wave damping theory accounting for thermal misbalance, explaining observed damping behaviors and revealing properties of coronal heating processes.
Findings
Modified damping relationship is not a power-law.
The model explains observed damping time scaling with wave period.
Seismologically constrains coronal heating mechanisms.
Abstract
Being directly observed in the Doppler shift and imaging data and indirectly as quasi-periodic pulsations in solar and stellar flares, slow magnetoacoustic waves offer an important seismological tool for probing many vital parameters of the coronal plasma. A recently understood active nature of the solar corona for magnetoacoustic waves, manifested through the phenomenon of wave-induced thermal misbalance, led to the identification of new natural mechanisms for the interpretation of observed properties of waves. A frequency-dependent damping of slow waves in various coronal plasma structures remains an open question, as traditional wave damping theories fail to match observations. We demonstrate that accounting for the back-reaction caused by thermal misbalance on the wave dynamics leads to a modification of the relationship between the damping time and oscillation period of standing…
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