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Coronal loops: observations and modeling of confined plasma
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 …
Coronal waves and oscillations
Wave and oscillatory activity of the solar corona is confidently observed with modern
imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and …
imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and …
Magnetohydrodynamic waves and coronal seismology: an overview of recent results
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 …
Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …
photosphere and the intensely heated transition region and corona. Compressible and …
Coronal loop oscillations-An interpretation in terms of resonant absorption of quasi-mode kink oscillations
Damped quasi-mode kink oscillations in cylindrical flux tubes are capable of explaining the
observed rapid dam** of the coronal loop oscillations when the ratio of the inhomogeneity …
observed rapid dam** of the coronal loop oscillations when the ratio of the inhomogeneity …
Resonant MHD waves in the solar atmosphere
The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The
review starts from discussing the properties of driven resonant MHD waves. The dissipative …
review starts from discussing the properties of driven resonant MHD waves. The dissipative …
Wave heating of the solar atmosphere
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 …
Time–distance seismology of the solar corona with CoMP
We employ a sequence of Doppler images obtained with the Coronal Multi-channel
Polarimeter (CoMP) instrument to perform time–distance seismology of the solar corona. We …
Polarimeter (CoMP) instrument to perform time–distance seismology of the solar corona. We …
Characteristics of transverse oscillations in a coronal loop arcade
TRACE observations from 15 April 2001 of transverse oscillations in coronal loops of a post-
flare loop arcade are investigated. They are considered to be standing fast kink oscillations …
flare loop arcade are investigated. They are considered to be standing fast kink oscillations …
Persistent Doppler shift oscillations observed with Hinode/EIS in the solar corona: spectroscopic signatures of Alfvénic waves and recurring upflows
Using data obtained by the EUV Imaging Spectrometer on board Hinode, we have
performed a survey of obvious and persistent (without significant dam**) Doppler shift …
performed a survey of obvious and persistent (without significant dam**) Doppler shift …