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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 …
Decoding the pre-eruptive magnetic field configurations of coronal mass ejections
A clear understanding of the nature of the pre-eruptive magnetic field configurations of
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …
Resolving the solar prominence/filament paradox using the magnetic Rayleigh–Taylor instability
Prominences and filaments are manifestations of magnetized, levitated plasma within the
solar coronal atmosphere. Their structure is assumed to be driven by the ambient magnetic …
solar coronal atmosphere. Their structure is assumed to be driven by the ambient magnetic …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
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 …
Simulations of solar filament fine structures and their counterstreaming flows
Solar filaments, also called solar prominences when appearing above the solar limb, are
cold, dense materials suspended in the hot tenuous solar corona, consisting of numerous …
cold, dense materials suspended in the hot tenuous solar corona, consisting of numerous …
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 …
Three-dimensional velocity fields of the solar filament eruptions detected by CHASE
The eruption of solar filaments, also known as prominences appearing off limb, is a common
phenomenon in the solar atmosphere. It ejects massive plasma and high-energy particles …
phenomenon in the solar atmosphere. It ejects massive plasma and high-energy particles …