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 …
Multi-scale variability of coronal loops set by thermal non-equilibrium and instability as a probe for coronal heating
Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
Polarisation of decayless kink oscillations of solar coronal loops
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 …
the enigmatic problem of solar and stellar coronal heating. The polarisation of the …
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 …
30-min decayless kink oscillations in a very long bundle of solar coronal plasma loops
The energy balance in the corona of the Sun is the key to the long-standing coronal heating
dilemma, which could be potentially revealed by observational studies of decayless kink …
dilemma, which could be potentially revealed by observational studies of decayless kink …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
B De Pontieu, P Testa, J Martínez-Sykora… - The Astrophysical …, 2022 - iopscience.iop.org
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 …
Transverse oscillations and an energy source in a strongly magnetized sunspot
D Yuan, L Fu, W Cao, B Kuźma, M Geeraerts… - Nature …, 2023 - nature.com
The solar corona is two to three orders of magnitude hotter than the underlying photosphere,
and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over …
and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over …
A statistical study of short-period decayless oscillations of coronal loops in an active region
Coronal loop oscillations are common phenomena in the solar corona, which are often
classified as decaying and decayless oscillations. Using the high-resolution observation …
classified as decaying and decayless oscillations. Using the high-resolution observation …