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Solar prominences: theory and models: Fleshing out the magnetic skeleton
Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot
corona. A comprehensive understanding of solar prominences ultimately requires complex …
corona. A comprehensive understanding of solar prominences ultimately requires complex …
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 european solar telescope
CQ Noda, R Schlichenmaier, LRB Rubio… - Astronomy & …, 2022 - aanda.org
The European Solar Telescope (EST) is a project aimed at studying the magnetic
connectivity of the solar atmosphere, from the deep photosphere to the upper …
connectivity of the solar atmosphere, from the deep photosphere to the upper …
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 …
Solar prominence diagnostics from non-LTE modelling of Mg II h&k line profiles
Aims. We investigate a new method to for obtaining the plasma parameters of solar
prominences observed in the Mg II h&k spectral lines by comparing line profiles from the …
prominences observed in the Mg II h&k spectral lines by comparing line profiles from the …
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 …
Mg II h&k fine structure prominence modelling and the consequences for observations
Aims. Using 2D Mg II h&k solar prominence modelling, our aim is to understand the
formation of complex line profiles and how these are seen by the Interface Region Imaging …
formation of complex line profiles and how these are seen by the Interface Region Imaging …
Spectro-imagery of an active tornado-like prominence: Formation and evolution
Context. The dynamical nature of fine structures in prominences remains an open issue,
including rotating flows in tornado prominences. While the Atmospheric Imaging Assembly …
including rotating flows in tornado prominences. While the Atmospheric Imaging Assembly …