Coronal loops: observations and modeling of confined plasma
F Reale - Living Reviews in Solar Physics, 2014 - Springer
Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …
brightness to the dense confined plasma, and this review focuses on loops mostly as …
Magnetohydrodynamic waves and coronal seismology: an overview of recent results
I De Moortel, VM Nakariakov - … Transactions of the …, 2012 - royalsocietypublishing.org
Recent observations have revealed that magnetohydrodynamic (MHD) waves and
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …
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 …
Standing slow-mode waves in hot coronal loops: observations, modeling, and coronal seismology
T Wang - Space science reviews, 2011 - Springer
Strongly damped Doppler shift oscillations are observed frequently associated with flarelike
events in hot coronal loops. In this paper, a review of the observed properties and the …
events in hot coronal loops. In this paper, a review of the observed properties and the …
Detection of the second harmonic of decay-less kink oscillations in the solar corona
T Duckenfield, SA Anfinogentov… - The Astrophysical …, 2018 - iopscience.iop.org
EUV observations of a multi-thermal coronal loop, taken by the Atmospheric Imaging
Assembly of the Solar Dynamics Observatory, which exhibits decay-less kink oscillations are …
Assembly of the Solar Dynamics Observatory, which exhibits decay-less kink oscillations are …
Novel data analysis techniques in coronal seismology
We review novel data analysis techniques developed or adapted for the field of coronal
seismology. We focus on methods from the last ten years that were developed for extreme …
seismology. We focus on methods from the last ten years that were developed for extreme …
Coronal loop seismology using damping of standing kink oscillations by mode coupling
Context. Kink oscillations of solar coronal loops are frequently observed to be strongly
damped. The damping can be explained by mode coupling on the condition that loops have …
damped. The damping can be explained by mode coupling on the condition that loops have …
Slow-mode magnetoacoustic waves in coronal loops
Rapidly decaying long-period oscillations often occur in hot coronal loops of active regions
associated with small (or micro-) flares. This kind of wave activity was first discovered with …
associated with small (or micro-) flares. This kind of wave activity was first discovered with …
Coronal loop seismology using damping of standing kink oscillations by mode coupling-II. additional physical effects and Bayesian analysis
Context. The strong damping of kink oscillations of coronal loops can be explained by mode
coupling. The damping envelope depends on the transverse density profile of the loop …
coupling. The damping envelope depends on the transverse density profile of the loop …
Coronal Alfvén speed determination: Consistency between seismology using AIA/SDO transverse loop oscillations and magnetic extrapolation
E Verwichte, T Van Doorsselaere… - The Astrophysical …, 2013 - iopscience.iop.org
Two transversely oscillating coronal loops are investigated in detail during a flare on the
2011 September 6 using data from the Atmospheric Imaging Assembly (AIA) on board the …
2011 September 6 using data from the Atmospheric Imaging Assembly (AIA) on board the …