Physics of Solar Prominences: II - Magnetic Structure and Dynamics

Abstract

Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them.

75 pages, 31 pictures, review paper

References in corpus (14)

• Physics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling
• The Emergence of a Twisted Flux Tube into the Solar Atmosphere: Sunspot Rotations and the Formation of a Coronal Flux Rope
• Emergence of a Helical Flux Rope Under an Active Region Prominence
• Eruption of magnetic flux ropes during flux emergence
• Modelling the Global Solar Corona: Filament Chirality Observations and Surface Simulations
• Transverse oscillations of flowing prominence threads observed with Hinode
• The effect of the relative orientation between the coronal field and new emerging flux: I Global Properties
• Prominence Formation Associated with an Emerging Helical Flux Rope
• Damping of Fast Magnetohydrodynamic Oscillations in Quiescent Filament Threads
• Non-adiabatic magnetohydrodynamic waves in a cylindrical prominence thread with mass flow
• Nonlinear force-free models for the solar corona I. Two active regions with very different structure
• Modelling the Global Solar Corona III: Origin of the Hemispheric Pattern of Filaments
• Evolution and Distribution of Current Helicity in Full-Sun Simulations
• Large-scale horizontal flows in the solar photosphere III: Effects on filament destabilization

Cited by in corpus (294)

• Physics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling
• Evolution of Magnetic Field and Energy in A Major Eruptive Active Region Based on SDO/HMI Observation
• Flare-productive active regions
• Magnetic Properties of Solar Active Regions that Govern Large Solar Flares and Eruptions
• The Magnetic Field in the Solar Atmosphere
• Partially Ionized Plasmas in Astrophysics
• Formation and evolution of a multi-threaded prominence
• Solar science with the Atacama Large Millimeter/submillimeter Array - A new view of our Sun
• Decoding the Pre-Eruptive Magnetic Field Configurations of Coronal Mass Ejections
• A solar tornado observed by AIA/SDO: Rotational flow and evolution of magnetic helicity in a prominence and cavity
• Origin and Structures of Solar Eruptions I: Magnetic Flux Rope (Invited Review)
• Simulations of Prominence Formation in the Magnetized Solar Corona by Chromospheric Heating
• Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. I- Observational aspects
• Large Amplitude Longitudinal Oscillations in a Solar Filament
• Formation of Solar Filaments by Steady and Nonsteady Chromospheric Heating
• Imaging and Spectroscopic Observations of a Filament Channel and the Implications for the Nature of Counter-streamings
• Numerical Investigation of a Coronal Mass Ejection from an Anemone Active Region: Reconnection and Deflection of the 2005 August 22 Eruption
• Solar Magnetized "Tornadoes": Relation to Filaments
• Initiation and Early Kinematic Evolution of Solar Eruptions
• An active region filament studied simultaneously in the chromosphere and photosphere: I - Magnetic structure
• Observations and Magnetic Field Modeling of a Solar Polar Crown Prominence
• The European Solar Telescope
• Observations and Implications of Large-Amplitude Longitudinal Oscillations in a Solar Filament
• Velocity vectors of a quiescent prominence observed by Hinode/SOT and the MSDP (Meudon)
• Magnetic Flux Ropes in the Solar Corona: Structure and Evolution toward Eruption
• On the Relationship Between a Hot-channel-like Solar Magnetic Flux Rope and its embedded Prominence
• SDO/AIA Observations of Large-Amplitude Longitudinal Oscillations in a Solar Filament
• The discovery of geomagnetically trapped cosmic ray antiprotons
• SDO/AIA Detection of Solar Prominence Formation within a Coronal Cavity
• Magnetic Structure and Dynamics of the Erupting Solar Polar Crown Prominence on 2012 March 12
• Multiwavelength observations of a partially eruptive filament on 2011 September 8
• The effects of magnetic-field geometry on longitudinal oscillations of solar prominences
• Rayleigh-Taylor instability in prominences from numerical simulations including partial ionization effects
• Open questions on prominences from coordinated observations by IRIS, Hinode, SDO/AIA, THEMIS, and the Meudon/MSDP
• A solar tornado triggered by flares?
• Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse
• Imaging and Spectroscopic Diagnostics on the Formation of Two Magnetic Flux Ropes Revealed by SDO/AIA and IRIS
• Parametric survey of longitudinal prominence oscillation simulations
• Simulations of solar filament fine structures and their counterstreaming flows
• Flux-Rope Twist in Eruptive Flares and CMEs: due to Zipper and Main-Phase Reconnection
• The magnetic field configuration of a solar prominence inferred from spectropolarimetric observations in the He I 10830 A triplet
• Magnetic fields of an active region filament from full Stokes analysis of Si I 1082.7 nm and He I 1083.0 nm
• Anti-parallel EUV flows observed along active region filament threads with Hi-C
• Stereoscopic Observations of an Erupting Mini-filament Driven Two-Sided-Loop Jet and the Applications for Diagnosing Filament Magnetic field
• GONG Catalog of Solar Filament Oscillations Near Solar Maximum
• The Birth of A Coronal Mass Ejection
• Polarimetric Properties of Flux-Ropes and Sheared Arcades in Coronal Prominence Cavities
• Evidence for rotational motions in the feet of a quiescent solar prominence
• Reconnection-Condensation Model for Solar Prominence Formation
• Numerical Simulations of the Magnetic Rayleigh-Taylor Instability in the Kippenhahn-Schlüter Prominence Model
• Simultaneous transverse and longitudinal oscillations in a quiescent prominence triggered by a coronal jet
• Witnessing tether-cutting reconnection at the onset of a partial eruption
• Statistical Analysis of Filament Features Based on the Hα Solar Images from 1988 to 2013 by Computer Automated Detection Method
• Why torus-unstable solar filaments experience failed eruption?
• Chirality of High Latitude Filaments over Solar Cycle 23
• Electric-Current Neutralization, Magnetic Shear, and Eruptive Activity in Solar Active Regions
• First direct observation of a torsional Alfvén oscillation at coronal heights
• The formation of an inverse S-shaped active-region filament driven by sunspot motion and magnetic reconnection
• On the Characteristics of Footpoints of Solar Magnetic Flux Ropes during the Eruption
• Coronal Quasi-periodic Fast-mode Propagating Wave Trains
• Large-Amplitude Longitudinal Oscillations Triggered by the Merging of Two Solar Filaments: Observations and Magnetic Field Analysis
• Spectro-polarimetric Imaging Reveals Helical Magnetic Fields in Solar Prominence Feet
• Quiescent prominence dynamics observed with the Hinode Solar Optical Telescope . II. Prominence Bubble Boundary Layer Characteristics and the Onset of a Coupled Kelvin-Helmholtz Rayleigh-Taylor Instability
• Triggering mechanism and material transfer of a failed solar filament eruption
• The origin of net electric currents in solar active regions
• An active region filament studied simultaneously in the chromosphere and photosphere. II. Doppler velocities
• Prominence formation by levitation-condensation at extreme resolutions
• Tether-cutting Reconnection between Two Solar Filaments Triggering Outflows and a Coronal Mass Ejection
• Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST
• Rayleigh-Taylor instability in partially ionized compressible plasmas: one fluid approach
• Thermal instabilities: Fragmentation and field misalignment of filament fine structure
• Double-Decker Filament Configuration Revealed by Mass Motions
• Unambiguous Evidence of Filament Splitting-Induced Partial Eruptions
• Filament Channel Formation Via Magnetic Helicity Condensation
• The Hydromagnetic Interior of a Solar Quiescent Prominence. I. Coupling between Force-balance and Steady Energy-transport
• Understanding the Role of Mass-Unloading in Filament Eruptions
• Can we explain non-typical solar flares?
• A Comprehensive Radiative Magnetohydrodynamics Simulation of Active Region Scale Flux Emergence from the Convection Zone to the Corona
• Magnetic field in atypical prominence structures: Bubble, tornado and eruption
• The 3D structure of an active region filament as extrapolated from photospheric and chromospheric observations
• Is flux rope a necessary condition for the progenitor of coronal mass ejections?
• Structure of prominence legs: Plasma and magnetic field
• Formation of an active region filament driven by a series of jets
• Observational detection of drift velocity between ionized and neutral species in solar prominences
• Non-equilibrium Flux Rope Formation by Confined Flares Preceding a Solar Coronal Mass Ejection
• The Origin of Solar Filament Plasma Inferred from in situ Observations of Elemental Abundances
• Observations of the Kelvin-Helmholtz instability driven by dynamic motions in a solar prominence
• Modeling a Carrington-scale Stellar Superflare and Coronal Mass Ejection from ${\kappa }^{1}Cet$
• Large-amplitude longitudinal oscillations in a solar filament
• Solar prominences embedded in flux ropes: morphological features and dynamics from 3D MHD simulations
• Two Step Filament Eruption During 14-15 March 2015
• Successive Homologous Coronal Mass Ejections driven by shearing and converging motions in solar active region NOAA 12371
• Damping mechanisms for oscillations in solar prominences
• Triggering an eruptive flare by emerging flux in a solar active-region complex
• Turbulent characteristics in the intensity fluctuations of a solar quiescent prominence observed by the \textit{Hinode} Solar Optical Telescope
• Tilt Angles of Solar Filaments over the Period 1919-2014
• Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions
• Dependence of the Length of Solar Filament Threads on the Magnetic Configuration
• Oscillatory motions observed in eruptive filaments
• Sunspot splitting triggering an eruptive flare
• Counter-streaming flows in a giant quiet-Sun filament observed in the extreme ultraviolet
• Longitudinal filament oscillations enhanced by two C-class flares
• Formation and material supply of an active-region filament associated with newly emerging flux
• A unified model of solar prominence formation
• First High-resolution Spectroscopic Observations of an Erupting Prominence Within a Coronal Mass Ejection by the Interface Region Imaging Spectrograph (IRIS)
• Coronal Mini-jets in an Activated Solar Tornado-like Prominence
• Material supply and magnetic configuration of an active region filament
• The influence of flux rope heating models on solar prominence formation
• Helical motions of fine-structure prominence threads observed by Hinode and IRIS
• The Mechanism for the Energy Buildup Driving Solar Eruptive Events
• A giant quiescent solar filament observed with high-resolution spectroscopy
• Magnetic Twists of Solar Filaments
• A Universal Method for Solar Filament Detection from H-alpha Observations using Semi-supervised Deep Learning
• Vertical oscillation of a coronal cavity triggered by an EUV wave
• Anomalous circular polarization profiles in the He I 1083.0 nm multiplet from solar spicules
• On magnetic reconnection and flux rope topology in solar flux emergence
• External reconnection and resultant reconfiguration of overlying magnetic fields during sympathetic eruptions of two filaments
• Spatial Damping of Propagating Kink Waves in Prominence Threads
• Simultaneous longitudinal and transverse oscillation in an active filament
• Sympathetic Filament Eruptions within a Fan-spine Magnetic System
• Oscillations and mass-draining that lead to a sympathetic eruption of a quiescent filament
• Modeling a Coronal Mass Ejection from an Extended Filament Channel. I. Eruption and Early Evolution
• Field topologies in ideal and near ideal magnetohydrodynamics and vortex dynamics
• Spectroscopic and imaging observations of small-scale reconnection events
• Numerical simulations of large-amplitude oscillations in flux-rope solar prominences
• Spectroscopic and Stereoscopic Observations of the Solar Jets
• Network Jets as the Driver of Counter-Streaming Flows in a Solar Filament/Filament Channel
• Filament Eruption and Its Reformation Caused by Emerging Magnetic Flux
• Formation of a Solar Filament by Magnetic Reconnection and Associated Chromospheric Evaporation and Subsequent Coronal Condensation
• Toward detailed prominence seismology - I. Computing accurate 2.5D magnetohydrodynamic equilibria
• Magnetic Flux Rope Identification and Characterization from Observationally-Driven Solar Coronal Models
• Large-amplitude prominence oscillations following the impact by a coronal jet
• Formation of a Magnetic Flux Rope in the Early Emergence Phase of NOAA Active Region 12673
• Dissipative instability in partially ionised prominence plasmas
• Halpha Doppler shifts in a tornado in the solar corona
• Stereoscopic Observation of Simultaneous Longitudinal and Transverse Oscillations in a Single Filament Driven by Two-sided-loop Jet
• Eruptions from coronal bright points: A spectroscopic view by IRIS of a mini-filament eruption, QSL reconnection, and reconnection-driven outflows
• Determining the dynamics and magnetic fields in He I 10830 Å during a solar filament eruption
• Solar prominence diagnostics from non-LTE modelling of Mgii h&k line profiles
• High resolution observations of sympathetic eruptions by NVST
• Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes
• Fine-scale structures and material flows of quiescent filaments observed by New Vacuum Solar Telescope
• Determination of Prominence Plasma Beta from the Dynamics of Rising Plumes
• Persistent fast kink magnetohydrodynamic waves detected in a quiescent prominence
• Impact of Dynamic State on the Mass Condensation Rate of Solar Prominences
• The Solar Corona during the Total Eclipse on 16 June 1806: Graphical Evidence of the Coronal Structure during the Dalton Minimum
• Diagnostic potential of the Ca II 8542A line for solar filaments
• A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. I. Unusual History of an Eruptive Filament
• Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI Data
• A revised cone model and its application to non-radial prominence eruptions
• Hot prominence detected in the core of a Coronal Mass Ejection: III. Plasma filling factor from UVCS Lyman-$\alpha$ and Lyman-$\beta$ observations
• Toward detailed prominence seismology - II. Charting the continuous magnetohydrodynamic spectrum
• Legolas: a modern tool for magnetohydrodynamic spectroscopy
• An Observational Study of a "Rosetta-Stone" Solar Eruption
• Magnetic Field Modeling of hot channels in Four Flare/CME Events
• Binary-induced magnetic activity? Time-series echelle spectroscopy and photometry of HD123351 = CZ CVn
• Dynamic formation of multi-threaded prominences in arcade configurations
• Prominence Activation by Coronal Fast Mode Shock
• Quiescent and Eruptive Prominences at Solar Minimum: A Statistical Study via an Automated Tracking System
• 1.5D NLTE spectral synthesis of a 3D filament/prominence simulation
• EUV lines observed with EIS/Hinode in a solar prominence
• Dynamics evolution of a solar active-region filament from quasi-static state to eruption: rolling motion, untwisting motion, material transfer, and chirality
• The Role of Magnetic Helicity in Coronal Heating
• A partial filament eruption in three steps induced by external magnetic reconnection
• 3D numerical simulations of oscillations in solar prominences
• Decayless longitudinal oscillations of a solar filament maintained by quasi-periodic jets
• Spectro-imagery of an active tornado-like prominence: formation and evolution
• Modeling Repeatedly Flaring $\delta$ Sunspots
• The Thermal Instability of Solar Prominence Threads
• Interchange reconnection associated with a confined filament eruption: Implications for the source of transient cold-dense plasma in solar winds
• Synthetic hydrogen spectra of prominence oscillations
• Spectropolarimetric analysis of an active region filament. II. Evidence of the limitations of a single component model
• Damped kink oscillations of flowing prominence threads
• Simultaneous longitudinal and transverse oscillations in filament threads after a failed eruption
• Genesis and Coronal-jet-generating Eruption of a Solar Minifilament Captured by IRIS Slit-raster Spectra
• DeFiNe: an optimisation-based method for robust disentangling of filamentous networks
• Observations of a prominence eruption and loop contraction
• Magnetic Structure of an Erupting Filament
• Statistical analysis of UV spectra of a quiescent prominence observed by IRIS
• Characteristics and applications of interplanetary coronal mass ejection composition
• Disintegration of an Eruptive Filament via Interactions with Quasi-Separatrix Layers
• Filament Activation in Response to Magnetic Flux Emergence and Cancellation in Filament Channels
• The Formation of a Small-scale Filament after Flux Emergence on the Quiet Sun
• Prominence eruption initiated by helical kink-instability of an embedded flux rope
• Time evolution of plasma parameters during the rise of a prominence instability
• Magnetic separatrix as the source region of the plasma supply for an active-region filament
• Flux Rope Formation Due to Shearing and Zipper Reconnection
• On-disk solar coronal condensations facilitated by magnetic reconnection between open and closed magnetic structures
• 2D non-LTE modelling of a filament observed in the H_alpha line with the DST/IBIS spectropolarimeter
• Reconfiguration and eruption of a solar filament by magnetic reconnection with an emerging magnetic field
• Sympathetic eruptions of two filaments with an identifiable causal link observed by the Solar Dynamics Observatory
• Two Classes of Eruptive Events During Solar Minimum
• Solar Active Region Electric Currents Before and During Eruptive Flares
• Properties of a Small-scale Short-duration Solar Eruption with a Driven Shock
• On the structure and evolution of a polar crown prominence/filament system
• How eruptions of a small filament feed materials to a nearby larger-scaled filament
• Interaction of Two Filament Channels of Different Chiralities
• Two Types of Long-duration Quasi-static Evolution of Solar Filaments
• Finite amplitude transverse oscillations of a magnetic rope
• Plasmoid-fed prominence formation (PF${}^2$) during flux rope eruption
• MHD Seismology of a loop-like filament tube by observed kink waves
• Measuring three-dimensional shapes of stable solar prominences using stereoscopic observations from SDO and STEREO
• Chromospheric Synoptic Maps of Polar Crown Filaments
• Pre-eruption Splitting of the Double-Decker Structure in a Solar Filament
• Observations of upward propagating waves in the transition region and corona above Sunspots
• Observations of apparent superslow wave propagation in solar prominences
• Intrusion of Magnetic Peninsula toward the Neighboring Opposite-polarity Region That Triggers the Largest Solar Flare in Solar Cycle 24
• Unified Relationship between Cold Plasma Ejections and Flare Energies Ranging from Solar Microflares to Giant Stellar Flares
• On the partial eruption of a bifurcated solar filament structure
• Current sheets in the wake of an eruption of two crossing filaments
• Erupting filaments with large enclosing flux tubes as sources of high-mass 3-part CMEs, and erupting filaments in the absence of enclosing flux tubes as sources of low-mass unstructured CMEs
• Dynamics of a solar prominence tornado observed by SDO/AIA on 2012 November 7-8
• Destabilization of a Solar Prominence/Filament Field System by a Series of Eight Homologous Eruptive Flares
• Formation of Quiescent Prominence Magnetic Field by Supergranulations
• Filament Shape Versus Coronal Potential Magnetic Field Structure
• Stability of the coronal magnetic field around large confined and eruptive solar flares
• Filament Eruption Driving EUV Loop Contraction then Expansion above a Stable Filament
• Rapid Rotation of an Erupting Prominence and the Associated Coronal Mass Ejection on 13 May 2013
• Formation of a solar filament by magnetic reconnection and coronal condensation
• A 7~MK hot Flux Rope Observed by SDO/AIA
• Untwisting and Disintegration of a Solar Filament Associated with Photospheric Flux Cancellation
• Formation of a solar Ha filament from orphan penumbrae
• Failed Solar Eruption of A Multi-thermal Flux Rope
• Interaction of solar jets with filaments: Triggering of large-amplitude filament oscillations
• Dynamics of descending knots in a solar prominence and their possible contributions to the heating of the local corona
• Winking filaments due to cyclic evaporation-condensation
• A formation mechanism for the large plumes in the prominence
• Large-Scale Vortex Motion and Multiple Plasmoid Ejection Due to Twisting Prominence Threads and Associated Reconnection
• Mass motion in a prominence bubble revealing a kinked flux rope configuration
• Reconstructing 3D Magnetic Topology of On-disk Prominence Bubbles from Stereoscopic Observations
• Twisting/Swirling Motions During a Prominence Eruption as seen from SDO/AIA
• Sequential Lid Removal in a Triple-Decker Chain of CME-Producing Solar Eruptions
• Solar Magnetic Fields
• Eruptions from coronal hole bright points: observations and non-potential modelling
• Association between Tornadoes and Instability of Hosting Prominence
• A Study of a long duration B9 flare-CME event and associated piston-driven shock
• Gravitational instability of solar prominence threads I. Curved magnetic fields without dips
• Stellar Differential Rotation and Coronal Timescales
• Does a solar filament barb always correspond to a prominence foot?
• Exploration of long-period oscillations in an H$\alpha$ prominence
• High-resolution Observation of Downflows at One End of a Pre-eruption Filament
• Buildup of the Magnetic Flux Ropes in Homologous Solar Eruptions
• Inference of magnetic fields in inhomogeneous prominences
• A Magnetic Bald-Patch Flare in Solar Active Region 11117
• Understanding the plasma and magnetic field evolution of a filament using observations and Nonlinear force-free field modelling
• Simulating Rayleigh-Taylor induced magnetohydrodynamic turbulence in prominences
• Radiative Magnetohydrodynamic Simulation of the Confined Eruption of a Magnetic Flux Rope: Magnetic Structure and Plasma Thermodynamics
• Heating of quiescent coronal loops caused by nearby eruptions observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager
• High-resolution spectroscopy of an erupting minifilament and its impact on the nearby chromosphere
• Modelling the magnetic structure of a large-scale horse-shoe-like filament in a decaying and diffuse active region
• Formation and Eruption of Hot Channels during an M6.5 Class Solar Flare
• Velocities of an Erupting Filament
• Performance Testing of an Off-Limb Solar Adaptive Optics System
• A Comparison Study of a Solar Active-Region Eruptive Filament and a Neighboring Non-Eruptive Filament
• The Astrophysical Variance in Gaia-RVS Spectra
• Crossing Filaments
• Properties of Magnetic Neutral Line Gradients and Formation of Filaments
• Hot prominence spicules launched from turbulent cool solar prominences
• The Role of a Tiny Brightening in a Huge Geo-effective Solar Eruption Leading to the St Patrick's Day Storm
• Synthetic radio views on simulated solar flux ropes
• Covert connection of filaments
• Two-horn quiescent prominence observed in H-alpha and MgII h&k lines with THEMIS and IRIS
• Sympathetic Quiet and Active Region Filament Eruptions
• Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths
• Spectral Characteristics of the He I D3 Line in a Quiescent Prominence Observed by THEMIS
• Future Prospects for Partially Ionised Solar Plasmas: the Prominence Case
• The He I 10830 A line: Radiative transfer and differential illumination effects
• Fast magnetohydrodynamic oscillation of longitudinally inhomogeneous prominence threads: an analogue with quantum harmonic oscillator
• Observations of Photospheric Vortical Motions During the Early Stage of Filament Eruption
• Filigree in the Surroundings of Polar Crown and High-Latitude Filaments
• A Three-Dimensional Velocity of an Erupting Prominence Prior to a Coronal Mass Ejection
• A giant dark channel across the solar equator consisting of two filament channels with different chiralities
• The Observations of Magnetic Reconnection During the Interaction Process of Two Active Region Filaments
• Evolution of photospheric flows under an erupting filament in the quiet-Sun region
• Shock-Cloud Interaction in the Solar Corona
• Solar Atmospheric Magnetic Energy Coupling: Broad Plasma Conditions and Spectrum Regimes
• Remote Sensing of Coronal Forces During a Solar Prominence Eruption
• Reconstruction of Coronal Magnetic Fields Using a Poloidal-Toroidal Representation
• Dynamics and connectivity of an extended arch filament system
• Observations of Photospheric Magnetic Structure below a Dark Filament using the Hinode Spectro-Polarimeter
• Effect of optically thin cooling curves on condensation formation: Case study using thermal instability
• Structure and dynamics of erupting solar prominences using the Rolling Hough Transform: Toward a feature-oriented classification
• Formation and Characteristics of Filament Threads in Double-Dipped Magnetic Flux Tubes
• Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions
• Falling Threads During Solar Filament Eruptions
• A first look into the magnetic field configuration of prominence threads using spectropolarimetric data
• Design of an adaptable Stokes polarimeter for exploring chromospheric magnetism
• Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption
• An analytical model of prominence dynamics
• The diversity of spectral shapes of hydrogen Lyman lines and Mg II lines in a quiescent prominence
• Reminiscences
• Energy release in the solar atmosphere from a stream of infalling prominence debris
• A Robust Deep Learning Framework for Prominence Detection through Composite Feature Representations
• Observational Study of Large Amplitude Longitudinal Oscillations in a Solar Filament