Quasi-periodic pulsations in solar and stellar flares: a review of underpinning physical mechanisms and their predicted observational signatures
The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been
known for over 50 years and significant progress has been made in this research area. It has …
known for over 50 years and significant progress has been made in this research area. It has …
Magnetohydrodynamic waves in the solar corona
VM Nakariakov, DY Kolotkov - Annual Review of Astronomy and …, 2020 - annualreviews.org
The corona of the Sun is a unique environment in which magnetohydrodynamic (MHD)
waves, one of the fundamental processes of plasma astrophysics, are open to a direct study …
waves, one of the fundamental processes of plasma astrophysics, are open to a direct study …
Coronal heating by MHD waves
The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …
the presence of ongoing heating that balances the strong radiative and thermal conduction …
Magnetohydrodynamic waves in open coronal structures
D Banerjee, S Krishna Prasad, V Pant… - Space Science …, 2021 - Springer
Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
The solar corona as an active medium for magnetoacoustic waves
DY Kolotkov, DI Zavershinskii… - Plasma Physics and …, 2021 - iopscience.iop.org
The presence and interplay of continuous cooling and heating processes maintaining the
corona of the Sun at the observed one million K temperature were recently understood to …
corona of the Sun at the observed one million K temperature were recently understood to …
Dispersion of slow magnetoacoustic waves in the active region fan loops introduced by thermal misbalance
SA Belov, NE Molevich, DI Zavershinskii - Solar Physics, 2021 - Springer
Slow magnetoacoustic waves observed in the solar corona are used as seismological
probes of plasma parameters. It has been shown that the dispersion properties of such …
probes of plasma parameters. It has been shown that the dispersion properties of such …
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability
BB Mikhalyaev, SB Derteev, NK Shividov… - Solar Physics, 2023 - Springer
In this article we study the properties of acoustic waves in the rarefied high-temperature
plasma of the solar corona, assuming that the heating and cooling of the plasma has a well …
plasma of the solar corona, assuming that the heating and cooling of the plasma has a well …
The effect of the magnetic field on the damping of slow waves in the solar corona
TJ Duckenfield, DY Kolotkov… - Astronomy & Astrophysics, 2021 - aanda.org
Context. Slow magnetoacoustic waves are routinely observed in astrophysical plasma
systems such as the solar corona, and they are usually seen to damp rapidly. As a slow …
systems such as the solar corona, and they are usually seen to damp rapidly. As a slow …
Role of non-ideal dissipation with heating–cooling misbalance on the phase shifts of standing slow magnetohydrodynamic waves
We analyse the phase shifts of standing, slow magnetohydrodynamic (MHD) waves in solar
coronal loops using a linear MHD model taking into account the role of thermal conductivity …
coronal loops using a linear MHD model taking into account the role of thermal conductivity …