Coronal waves and oscillations
VM Nakariakov, E Verwichte - Living Reviews in Solar Physics, 2005 - Springer
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 …
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 transverse magnetohydrodynamic waves in a solar prominence
Solar prominences are cool 104 kelvin plasma clouds supported in the surrounding 106
kelvin coronal plasma by as-yet-undetermined mechanisms. Observations from Hinode …
kelvin coronal plasma by as-yet-undetermined mechanisms. Observations from Hinode …
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 …
Hot coronal loop oscillations observed by SUMER: slow magnetosonic wave damping by thermal conduction
Recently, strongly damped Doppler shift oscillations of hot (T> 6 MK) coronal loops were
observed with the Solar Ultraviolet Measurement of Emitted Radiation (SUMER) …
observed with the Solar Ultraviolet Measurement of Emitted Radiation (SUMER) …
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 damping) Doppler shift …
performed a survey of obvious and persistent (without significant damping) Doppler shift …
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 …
How to channel photospheric oscillations into the corona
B De Pontieu, R Erdélyi, I De Moortel - The Astrophysical Journal, 2005 - iopscience.iop.org
There are now many observations of waves in the solar corona with periods around 5
minutes. The source of these waves is uncertain, although global p-modes in the …
minutes. The source of these waves is uncertain, although global p-modes in the …
Solar active regions: SOHO/CDS and TRACE observations of quiescent coronal loops
G Del Zanna, HE Mason - Astronomy & Astrophysics, 2003 - aanda.org
This study focuses on the diagnostic capabilities of the TRACE and SOHO-CDS instruments
to describe the physical characteristics of quiescent solar active regions. In particular we …
to describe the physical characteristics of quiescent solar active regions. In particular we …
The heating of the solar corona
RW Walsh, J Ireland - The Astronomy and Astrophysics Review, 2003 - Springer
The heating of the solar corona has been a fundamental astrophysical issue for over sixty
years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO …
years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO …