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 …
Review on current sheets in CME development: theories and observations
J Lin, NA Murphy, C Shen, JC Raymond… - Space Science …, 2015 - Springer
We introduce how the catastrophe model for solar eruptions predicted the formation and
development of the long current sheet (CS) and how the observations were used to …
development of the long current sheet (CS) and how the observations were used to …
The origin of underdense plasma downflows associated with magnetic reconnection in solar flares
Magnetic reconnection is a universal process that powers explosive energy-release events
such as solar flares, geomagnetic substorms and some astrophysical jets. A characteristic …
such as solar flares, geomagnetic substorms and some astrophysical jets. A characteristic …
Ultraviolet spectroscopy of the extended solar corona
JL Kohl, G Noci, SR Cranmer, JC Raymond - The Astronomy and …, 2006 - Springer
The first observations of ultraviolet spectral line profiles and intensities from the extended
solar corona (ie, more than 1.5 solar radii from Sun-center) were obtained on 13 April 1979 …
solar corona (ie, more than 1.5 solar radii from Sun-center) were obtained on 13 April 1979 …
Downflow motions associated with impulsive nonthermal emissions observed in the 2002 July 23 solar flare
A Asai, T YOkOYAMA, M Shimojo… - The Astrophysical …, 2004 - iopscience.iop.org
We present a detailed examination of downflow motions above flare loops observed in the
2002 July 23 flare. The extreme-ultraviolet images obtained with the Transition Region and …
2002 July 23 flare. The extreme-ultraviolet images obtained with the Transition Region and …
The 2014 March 29 X-flare: subarcsecond resolution observations of Fe XXI λ1354. 1
PR Young, H Tian, S Jaeggli - The Astrophysical Journal, 2015 - iopscience.iop.org
ABSTRACT The Interface Region Imaging Spectrometer (IRIS) is the first solar instrument to
observe∼ 10 MK plasma at subarcsecond spatial resolution through imaging spectroscopy …
observe∼ 10 MK plasma at subarcsecond spatial resolution through imaging spectroscopy …
X-ray sources and magnetic reconnection in the X3. 9 flare of 2003 November 3
Context. Recent RHESSI observations indicate an apparent altitude decrease of flare X-ray
loop-top (LT) sources before changing to the commonly observed upward growth of the flare …
loop-top (LT) sources before changing to the commonly observed upward growth of the flare …
Solar energetic particle charge states and abundances with nonthermal electrons
JY Lee, S Kahler, JC Raymond… - The Astrophysical …, 2024 - iopscience.iop.org
An important aspect of solar energetic particle (SEP) events is their source populations.
Elemental abundance enhancements of impulsive SEP events, originating in presumed …
Elemental abundance enhancements of impulsive SEP events, originating in presumed …
Imaging and spectroscopic observations of magnetic reconnection and chromospheric evaporation in a solar flare
Magnetic reconnection is believed to be the dominant energy release mechanism in solar
flares. The standard flare model predicts both downward and upward outflow plasmas with …
flares. The standard flare model predicts both downward and upward outflow plasmas with …
Hot plasma flows and oscillations in the loop-top region during the 2017 September 10 X8. 2 solar flare
In this study, we investigate motions in the hot plasma above the flare loops during the 2017
September 10 X8. 2 flare event. We examine the region to the south of the main flare arcade …
September 10 X8. 2 flare event. We examine the region to the south of the main flare arcade …