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Rayleigh–Taylor and Richtmyer–Meshkov instabilities: a journey through scales
Hydrodynamic instabilities such as Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM)
instabilities usually appear in conjunction with the Kelvin–Helmholtz (KH) instability and are …
instabilities usually appear in conjunction with the Kelvin–Helmholtz (KH) instability and are …
Origin and structures of solar eruptions I: magnetic flux rope
Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
Magnetic flux ropes in the solar corona: structure and evolution toward eruption
Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
Vortex motions in the solar atmosphere: Definitions, theory, observations, and modelling
Vortex flows, related to solar convective turbulent dynamics at granular scales and their
interplay with magnetic fields within intergranular lanes, occur abundantly on the solar …
interplay with magnetic fields within intergranular lanes, occur abundantly on the solar …
The magnetic Rayleigh–Taylor instability in solar prominences
A Hillier - Reviews of Modern Plasma Physics, 2017 - Springer
Abstract The magnetic Rayleigh–Taylor instability is a fundamental instability of many
astrophysical systems, and recent observations are consistent with this instability develo** …
astrophysical systems, and recent observations are consistent with this instability develo** …
1.5 D non-LTE spectral synthesis of a 3D filament and prominence simulation
Context. Overly idealised representations of solar filaments and prominences in numerical
simulations have long limited their morphological comparison against observations …
simulations have long limited their morphological comparison against observations …
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …
revolutionize our ability to measure, understand, and model the basic physical processes …
A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)
Abstract The Interface Region Imaging Spectrograph (IRIS) has been obtaining near-and far-
ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest …
ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest …
On the physical nature of the so-called prominence tornadoes
The term 'tornado'has been used in recent years to describe several solar phenomena, from
large-scale eruptive prominences to small-scale photospheric vortices. It has also been …
large-scale eruptive prominences to small-scale photospheric vortices. It has also been …
Quiescent Prominence Dynamics Observed with the Hinode Solar Optical Telescope. II. Prominence Bubble Boundary Layer Characteristics and the Onset of a …
We analyze solar quiescent prominence bubble characteristics and instability dynamics
using Hinode/Solar Optical Telescope data. We measure the bubble expansion rate …
using Hinode/Solar Optical Telescope data. We measure the bubble expansion rate …