Wave heating of the solar atmosphere
I Arregui - … Transactions of the Royal Society A …, 2015 - royalsocietypublishing.org
Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their
significance has increased because of their potential as a remote diagnostic tool and their …
significance has increased because of their potential as a remote diagnostic tool and their …
Longitudinal waves in coronal loops
I De Moortel - Space Science Reviews, 2009 - Springer
Outwardly propagating intensity disturbances are a common feature in large, quiescent
coronal loop structures. In this paper, an overview is given of the observed properties and …
coronal loop structures. In this paper, an overview is given of the observed properties and …
Damping of slow magnetoacoustic oscillations by the misbalance between heating and cooling processes in the solar corona
DY Kolotkov, VM Nakariakov… - Astronomy & …, 2019 - aanda.org
Context. Rapidly decaying slow magnetoacoustic waves are regularly observed in the solar
coronal structures, offering a promising tool for a seismological diagnostics of the coronal …
coronal structures, offering a promising tool for a seismological diagnostics of the coronal …
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 …
Observations of sausage modes in magnetic pores
We present here evidence for the observation of the magnetohydrodynamic (MHD) sausage
modes in magnetic pores in the solar photosphere. Further evidence for the omnipresent …
modes in magnetic pores in the solar photosphere. Further evidence for the omnipresent …
Hinode EUV spectroscopic observations of coronal oscillations
Context. Waves offer a unique opportunity to understand and diagnose the properties of the
solar coronal plasma. Aims. Hinode/EIS observations are analysed to detect wave and …
solar coronal plasma. Aims. Hinode/EIS observations are analysed to detect wave and …
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 …
Role of compressive viscosity and thermal conductivity on the damping of slow waves in coronal loops with and without heating–cooling imbalance
In the present article, we derive a new dispersion relation for slow magnetoacoustic waves
invoking the effect of thermal conductivity, compressive viscosity, radiation, and an unknown …
invoking the effect of thermal conductivity, compressive viscosity, radiation, and an unknown …
MHD wave propagation near coronal null points of magnetic fields
JA McLaughlin, AW Hood, I De Moortel - Space science reviews, 2011 - Springer
We present a comprehensive review of MHD wave behaviour in the neighbourhood of
coronal null points: locations where the magnetic field, and hence the local Alfvén speed, is …
coronal null points: locations where the magnetic field, and hence the local Alfvén speed, is …
Decayless low-amplitude transverse oscillations in short coronal loops as manifestations of driven slow modes
I Lopin, I Nagorny - Monthly Notices of the Royal Astronomical …, 2024 - academic.oup.com
ABSTRACT A recent theoretical study of slow magnetoacoustic oscillations in a curved
magnetic slab shows that the principal slow mode causes both dominant longitudinal …
magnetic slab shows that the principal slow mode causes both dominant longitudinal …