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. The unique combination of near and far-ultraviolet spectra and images at subarcsecond resolution and high cadence allows the tracing of mass and energy through the critical interface between the solar surface and the corona or solar wind. IRIS has enabled research into the fundamental physical processes thought to play a role in the low solar atmosphere such as ion-neutral interactions, magnetic reconnection, the generation, propagation, and dissipation of various types of waves, the acceleration of non-thermal particles, and various small-scale instabilities. These new findings have helped provide novel insights into a wide range of phenomena including the discovery of non-thermal particles in coronal nanoflares, the formation and impact of spicules and other jets, resonant absorption and dissipation of Alfvenic waves, energy release associated with braiding of magnetic field lines, the thermal instability in the chromosphere-corona mass and energy cycle, the contribution of waves, turbulence, and non-thermal particles in the energy deposition during flares and smaller-scale events such as UV bursts, and the role of flux ropes and other mechanisms in triggering CMEs. IRIS observations have also advanced studies of the connections between solar and stellar physics. Advances in numerical modeling, inversion codes, and machine learning techniques have played a key role in driving these new insights. With the advent of exciting new instrumentation both on the ground (e.g., DKIST, ALMA) and space-based (e.g., Parker Solar Probe, Solar Orbiter), we aim to review new insights based on IRIS observations or related modeling, and highlight some of the outstanding challenges that have been brought to the fore.

arXiv comment105 pages, 30 figures, accepted for publication in Solar Physics

References in corpus (382)

• The chemical composition of the Sun
• The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission
• A Model for Solar Coronal Mass Ejections
• The Interface Region Imaging Spectrograph (IRIS)
• The Solar Optical Telescope for the Hinode Mission: An Overview
• The Solar Orbiter mission -- Science overview
• An Observational Overview of Solar Flares
• The stellar atmosphere simulation code Bifrost
• On the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant Heliosphere
• Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars
• Heating of the Solar Chromosphere and Corona by Alfven Wave Turbulence
• The MUSCLES Treasury Survey I: Motivation and Overview
• Evolution of Magnetic Field and Energy in A Major Eruptive Active Region Based on SDO/HMI Observation
• Impulsive phase flare energy transport by large-scale Alfven waves and the electron acceleration problem
• Radiative Hydrodynamic Models of the Optical and Ultraviolet Emission from Solar Flares
• MHD Waves and Coronal Seismology: an overview of recent results
• Solar Coronal Jets: Observations, Theory, and Modeling
• Small-scale filament eruptions as the driver of solar coronal hole X-ray jets
• Hot Explosions in the Cool Atmosphere of the Sun
• Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere
• The FIP and Inverse FIP Effects in Solar and Stellar Coronae
• Numerical simulations of quiet Sun magnetism: On the contribution from a small-scale dynamo
• An Ab Initio Approach to the Solar Coronal Heating Problem
• Dynamic Fibrils are driven by Magnetoacoustic Shocks
• Time-Resolved Properties and Global Trends in dMe Flares from Simultaneous Photometry and Spectra
• A Unified Computational Model for Solar and Stellar Flares
• Magnetic Braking Formulation for Sun-Like Stars: Dependence on Dipole Field Strength and Rotation Rate
• High Resolution Observations and Modeling of Dynamic Fibrils
• Coronal heating by MHD waves
• The formation of IRIS diagnostics II. The formation of the Mg II h&k lines in the solar atmosphere
• A Comparison of Flare Forecasting Methods, I: Results from the "All-Clear" Workshop
• Extension of the MURaM radiative MHD code for coronal simulations
• Velocity Characteristics of Evaporated Plasma Using Hinode/EIS
• Convectively driven vortex flows in the Sun
• Approximations for radiative cooling and heating in the solar chromosphere
• Observing the fine structure of loops through high resolution spectroscopic observations of coronal rain with the CRISP instrument at the Swedish Solar Telescope
• A publicly available simulation of an enhanced network region of the Sun
• The Sun in Time: Activity and Environment
• Observations of ubiquitous compressive waves in the Sun's chromosphere
• Evidence of Non-Thermal Particles in Coronal Loops Heated Impulsively by Nanoflares
• On the generation of solar spicules and Alfvénic waves
• On-disk counterparts of type II spicules in the Ca II 854.2 nm and Halpha lines
• Abiotic O${}_2$ Levels on Planets around F, G, K, and M Stars: Possible False Positives for Life?
• Quantifying Spicules
• Propagating waves along spicules
• High Stellar FUV/NUV Ratio and Oxygen Contents in the Atmospheres of Potentially Habitable Planets
• Nonlinear Instability of kink oscillations due to shear motions
• Sun-as-a-star Observation of White-Light Flares
• Extreme UV quiet Sun brightenings observed by Solar Orbiter/EUI
• From coronal observations to MHD simulations, the building blocks for 3D models of solar flares
• Asteroseismology of solar-type stars
• The formation of IRIS diagnostics I. A quintessential model atom of Mg II and general formation properties of the Mg II h&k lines
• Non-equilibrium hydrogen ionization in 2D simulations of the solar atmosphere
• Plasma Jets and Eruptions in Solar Coronal Holes: a 3D flux emergence experiment
• Multiphase Gas and the Fractal Nature of Radiative Turbulent Mixing Layers
• Connecting Flares and Transient Mass Loss Events in Magnetically Active Stars
• From Radio to X-ray: Flares on the dMe Flare Star EV Lacertae
• Do Kepler superflare stars really include slowly-rotating Sun-like stars ? - Results using APO 3.5m telescope spectroscopic observations and Gaia-DR2 data -
• An Interface Region Imaging Spectrograph first view on Solar Spicules
• Radiative transfer with scattering for domain-decomposed 3D MHD simulations of cool stellar atmospheres
• Microflares and the Statistics of X-ray Flares
• The MUSCLES Treasury Survey. V. FUV Flares on Active and Inactive M Dwarfs
• On the prevalence of small-scale twist in the solar chromosphere and transition region
• Coronal rain as a marker for coronal heating mechanisms
• A HR-like Diagram for Solar/Stellar Flares and Corona -- Emission Measure vs Temperature Diagram
• Temporal evolution of multiple evaporating ribbon sources in a solar flare
• Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. II- Numerical aspects
• Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton
• The formation of IRIS diagnostics. III. Near-ultraviolet Spectra and Images
• Nonlinear propagation of Alfven waves driven by observed photospheric motions: Application to the coronal heating and spicule formation
• Temporal evolution of chromospheric evaporation: case studies of the M1.1 flare on 2014 September 6 and X1.6 flare on 2014 September 10
• High-resolution Observations of the Shock Wave Behavior for Sunspot Oscillations with the Interface Region Imaging Spectrograph
• Imaging and spectroscopic observations of magnetic reconnection and chromospheric evaporation in a solar flare
• Observing coronal nanoflares in active region moss
• Ellerman bombs at high resolution III. Simultaneous observations with IRIS and SST
• Bombs and flares at the surface and lower atmosphere of the Sun
• On active region loops: Hinode/EIS observations
• Slipping Magnetic Reconnection, Chromospheric Evaporation, Implosion, and Precursors in the 2014 September 10 X1.6-Class Solar Flare
• Magnetic Reconnection along Quasi-Separatrix Layers as a Driver of Ubiquitous Active Region Outflows
• Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. I- Observational aspects
• Radiative Hydrodynamic Models of Optical and Ultraviolet Emission from M Dwarf Flares
• Are IRIS bombs connected to Ellerman bombs?
• The multi-thermal and multi-stranded nature of coronal rain
• The Unresolved Fine Structure Resolved - IRIS observations of the Solar Transition Region
• Solar Magnetized "Tornadoes": Relation to Filaments
• Unprecedented Fine Structure of a Solar Flare Revealed by the 1.6~m New Solar Telescope
• Global sausage oscillation of solar flare loops detected by the Interface Region Imaging Spectrograph
• Homologous Helical Jets: Observations by IRIS, SDO and Hinode and Magnetic Modeling with Data-Driven Simulations
• Above-the-loop-top Oscillation and Quasi-periodic Coronal Wave Generation in Solar Flares
• Multiwavelength Observations of Small-Scale Reconnection Events triggered by Magnetic Flux Emergence in the Solar Atmosphere
• Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data
• The Formation of IRIS diagnostics. IV. The Mg II triplet lines as a new diagnostic for lower chromospheric heating
• Quasi-periodic Slipping Magnetic Reconnection During an X-class Solar Flare Observed by the Solar Dynamics Observatory and Interface Region Imaging Spectrograph
• Non-LTE inversions of the Mg II h&k and UV triplet lines
• Continuum Enhancements in the Ultraviolet, the Visible and the Infrared during the X1 flare on 2014 March 29
• Drifting of the line-tied footpoints of CME flux-ropes
• The height of a white-light flare and its hard X-ray sources
• A basal contribution from p-modes to the Alfvénic wave flux in the Sun's corona
• The Atmospheric Response to High Nonthermal Electron Beam Fluxes in Solar Flares I: Modeling the Brightest NUV Footpoints in the X1 Solar Flare of 2014 March 29
• Properties of a solar flare kernel observed by Hinode and SDO
• New Insights into White-Light Flare Emission from Radiative-Hydrodynamic Modeling of a Chromospheric Condensation
• The 2014 March 29 X-flare: sub-arcsecond resolution observations of Fe XXI 1354.1
• Simulations of the Mg II k and Ca II 8542 lines from an Alfvén Wave-heated flare chromosphere
• Iris si iv line profiles: An indication for the plasmoid instability during small-scale magnetic reconnection on the sun
• Frequently Occurring Reconnection Jets from Sunspot Light Bridges
• Overlapping Magnetic Activity Cycles and the Sunspot Number: Forecasting Sunspot Cycle 25 Amplitude
• Dynamics of solar coronal loops II. Catastrophic cooling and high-speed downflows
• Intermittent reconnection and plasmoids in UV bursts in the low solar atmosphere
• Multidimensional modeling of coronal rain dynamics
• Ellerman bombs and UV bursts: transient events in chromospheric current sheets
• The High-Energy Radiation Environment Around a 10 Gyr M Dwarf: Habitable at Last?
• HAZMAT. IV. Flares and Superflares on Young M Stars in the Far Ultraviolet
• Estimating the "Dark" Energy Content of the Solar Corona
• Three-dimensional Magnetohydrodynamic Simulation of the Formation of Solar Chromospheric Jets with Twisted Magnetic Field Lines
• Evidence for evaporation-incomplete condensation cycles in warm solar coronal loops
• Why one-dimensional models fail in the diagnosis of average spectra from inhomogeneous stellar atmospheres
• Why Is Non-thermal Line Broadening of Spectral Lines in The Lower Transition Region of the Sun Independent of Spatial Resolution?
• Far-Ultraviolet Activity Levels of F, G, K, and M dwarf Exoplanet Host Stars
• Numerical Simulations of Coronal Heating through Footpoint Braiding
• Benchmarking Fast-to-Alfven Mode Conversion in a Cold MHD Plasma
• Detection of supersonic downflows and associated heating events in the transition region above sunspots
• Propagation of Alfvénic Waves From Corona to Chromosphere and Consequences for Solar Flares
• Coronal-Jet-Producing Minifilament Eruptions as a Possible Source of Parker Solar Probe (PSP) Switchbacks
• Simultaneous IRIS and Hinode/EIS observations and modelling of the 27 October 2014 X 2.0 class flare
• Multiwavelength observations of a giant flare on CN Leonis I. The chromosphere as seen in the optical spectra
• Light Bridge in a Developing Active Region. I. Observation of Light Bridge and its Dynamic Activity Phenomena
• Data-driven Radiative Hydrodynamic Modeling of the 2014 March 29 X1.0 Solar Flare
• Heating signatures in the disk counterparts of solar spicules in IRIS observations
• Transverse oscillations of loops with coronal rain observed by Hinode/SOT
• Vortices in simulations of solar surface convection
• Spatially-Resolved Nonthermal Line Broadening During The Impulsive Phase of a Solar Flare
• Explosive Chromospheric Evaporation in a Circular-ribbon Flare
• Spectral signatures of chromospheric condensation in a major solar flare
• SDO/AIA Detection of Solar Prominence Formation within a Coronal Cavity
• Hydrogen Balmer Continuum in Solar Flares Detected by the Interface Region Imaging Spectrograph (IRIS)
• Magnetohydrodynamic Fast Sausage Waves in the Solar Corona
• Measurements of Absolute Abundances in Solar Flares
• M Dwarf Flare Continuum Variations on One-Second Timescales: Calibrating and Modeling of ULTRACAM Flare Color Indices
• H-alpha features with hot onsets. I. Ellerman bombs
• Identifying typical Mg II flare spectra using machine learning
• Recovering Thermodynamics from Spectral Profiles observed by IRIS: A Machine and Deep Learning Approach
• Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere
• Microflare Heating of a Solar Active Region Observed with NuSTAR, Hinode/XRT, and SDO/AIA
• Rayleigh-Taylor instability in prominences from numerical simulations including partial ionization effects
• Detailed and simplified non-equilibrium helium ionization in the solar atmosphere
• Chromospheric Condensation and Quasi-periodic Pulsations in a Circular-ribbon Flare
• What do iris observations of Mg II k tell us about the solar plage chromosphere?
• Investigating the response of loop plasma to nanoflare heating using RADYN simulations
• The cool surge following flux emergence in a radiation-MHD experiment
• The formation of IRIS diagnostics V. A quintessential model atom of C II and general formation properties of the C II lines at 133.5 nm
• Generalized phase mixing: Turbulence-like behaviour from unidirectionally propagating MHD waves
• Solar Transition-Region Lines Observed by the Interface Region Imaging Spectrograph: Diagnostics for the O IV and Si IV Lines
• Open questions on prominences from coordinated observations by IRIS, Hinode, SDO/AIA, THEMIS, and the Meudon/MSDP
• On the occurrence of thermal non-equilibrium in coronal loops
• The High-Resolution Coronal Imager, Flight 2.1
• Apparent Solar Tornado - Like Prominences
• Chromospheric Evaporation in an X1.0 Flare on 2014 March 29 Observed with IRIS and EIS
• Imaging and Spectroscopic Diagnostics on the Formation of Two Magnetic Flux Ropes Revealed by SDO/AIA and IRIS
• Si IV Resonance Line Emission During Solar Flares: Non-LTE, Non-equilibrium, Radiation Transfer Simulations
• Transverse Wave Induced Kelvin-Helmholtz Rolls in Spicules
• Stellar Activity and Coronal Heating: an overview of recent results
• Long-period intensity pulsations in the solar corona during activity cycle 23
• IRIS Observations of the Mg II h & k Lines During a Solar Flare
• The Near-Ultraviolet Continuum Radiation in the Impulsive Phase of HF/GF-Type dMe Flares I: Data
• Accelerated electrons observed down to <7 keV in a NuSTAR solar microflare
• Surges and Si IV bursts in the solar atmosphere. Understanding IRIS and SST observations through RMHD experiments
• Spectroscopic observations of evolving flare ribbon substructure suggesting origin in current sheet waves
• Mass Loss Rates from Coronal Mass Ejections: A Predictive Theoretical Model for Solar-Type Stars
• The fast filament eruption leading to the X-flare on March 29, 2014
• A method for global inversion of multi-resolution solar data
• Observations of Solar Coronal Rain in Null Point Topologies
• Damping of Alfven waves in solar partially ionized plasmas: effect of neutral helium in multi-fluid approach
• Magnetic reconnection at the earliest stage of solar flux emergence
• Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI
• Double arc instability in the solar corona
• First Detection of Plasmoids from Breakout Reconnection on the Sun
• Ion-neutral interactions and non-equilibrium ionization in the solar chromosphere
• Long-Period Intensity Pulsations in Coronal Loops Explained by Thermal Non-Equilibrium Cycles
• The development of lower-atmosphere turbulence early in a solar flare
• Density diagnostics derived from the OIV and SIV intercombination lines observed by IRIS
• Coronal condensations caused by magnetic reconnection between solar coronal loops
• Non-equilibrium helium ionization in an MHD simulation of the solar atmosphere
• Light Bridge in a Developing Active Region. II. Numerical Simulation of Flux Emergence and Light Bridge Formation
• Hi-C 2.1 Observations of Jetlet-like Events at Edges of Solar Magnetic Network Lane
• Evidence for rotational motions in the feet of a quiescent solar prominence
• Stellar Characterization of M-dwarfs from the APOGEE Survey: A Calibrator Sample for the M-dwarf Metallicities
• Observations and numerical models of solar coronal heating associated with spicules
• Explosive events in active region observed by IRIS and SST/CRISP
• Dynamics of coronal rain and descending plasma blobs in solar prominences: I. Fully ionised case
• Non-Maxwellian analysis of the transition-region line profiles observed by the Interface Region Imaging Spectrograph
• Blue wing enhancement of the chromospheric Mg II h and k lines in a solar flare
• Continuous upflows and sporadic downflows observed in active regions
• The first X-ray imaging spectroscopy of quiescent solar active regions with NuSTAR
• What the sudden death of solar cycles can tell us about the nature of the solar interior
• UV spectra, bombs, and the solar atmosphere
• Multi-episode chromospheric evaporation observed in a solar flare
• Impact of Type II Spicules in the Corona: Simulations and Synthetic Observables
• Oscillating light wall above a sunspot light bridge
• IRIS and SDO observation of recurrent explosive events
• HST/STIS High Resolution Echelle Spectra of alpha Centauri A (G2 V)
• Comparative Modelling of the Spectra of Cool Giants
• Vector magnetic field measurements along a cooled stereo-imaged coronal loop
• Ellerman bombs and UV bursts: reconnection at different atmospheric layers
• Hot Plasma Flows and Oscillations in the Loop-top Region During the September 10 2017 X8.2 Solar Flare
• The passband integrationproperties of Birefringent filter
• First direct observation of a torsional Alfvén oscillation at coronal heights
• Observing Kelvin-Helmholtz instability in solar blowout jet
• Observational Evidences of Electron-driven Evaporation in two Solar Flares
• How important are electron beams in driving chromospheric evaporation in the 2014 March 29 flare?
• What causes the high apparent speeds in chromospheric and transition region spicules on the Sun?
• Internetwork chromospheric bright grains observed with IRIS
• IRIS observations of short-term variability in moss associated with transient hot coronal loops
• IRIS Burst Spectra Co-Spatial To A Quiet-Sun Ellerman-Like Brightening
• Clusters of small eruptive flares produced by magnetic reconnection in the sun
• Transition Region and Chromospheric Signatures of Impulsive Heating Events. I. Observations
• A parameter study for modeling MgII h and k emission during solar flares
• High spatial resolution FeXII observations of solar active region
• 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
• Various Local Heating Events in the Earliest Phase of Flux Emergence
• Near-Ultraviolet Spectra of Flares on YZ CMi
• Amplitudes and energy fluxes of simulated decayless kink oscillations
• The Formation of IRIS Diagnostics. VII. The Formation of the OI 135.56 nm Line in the Solar Atmosphere
• Statistical study of network jets observed in the solar transition region: A comparison between coronal holes and quiet sun regions
• Evidence for a Transition Region response to penumbral microjets in sunspots
• Flame-like Ellerman Bombs and Their Connection to Solar UV Bursts
• A simple model of chromospheric evaporation and condensation driven conductively in a solar flare
• Properties of chromospheric evaporation and plasma dynamics of a solar flare from IRIS observations
• IRIS observations of magnetic interactions in the solar atmosphere between pre-existing and emerging magnetic fields. I. Overall evolution
• Propagating Disturbances in The Solar Corona and Spicular Connection
• A case-study of multi-temperature coronal jets for emerging flux MHD models
• On Kelvin-Helmholtz and parametric instabilities driven by coronal waves
• Cool transition region loops observed by the Interface Region Imaging Spectrograph
• A Hydrodynamic Model of Alfvénic Wave Heating in a Coronal Loop and its Chromospheric Footpoints
• Ultra-narrow Negative Flare Front Observed in Helium-10830~Å using the 1.6 m New Solar Telescope
• Subarcsecond blobs in flare-related coronal jets
• Modeling Mg II h, k and Triplet Lines at Solar Flare Ribbons
• Real-time flare prediction based on distinctions between flaring and non-flaring active region spectra
• Observational Evidence of Magnetic Reconnection for Brightenings and Transition Region Arcades in IRIS observations
• An observationally-constrained model of strong magnetic reconnection in the solar chromosphere. Atmospheric stratification and estimates of heating rates
• Observed Variability of the Solar Mg II h Spectral Line
• The cause of spatial structure in solar He I 1083 nm multiplet images
• Two-fluid simulations of waves in the solar chromosphere II. Propagation and damping of fast magneto-acoustic waves and shocks
• A secondary fan-spine magnetic structure in active region 11897
• Magnetic field in atypical prominence structures: Bubble, tornado and eruption
• Sun-Like Magnetic Cycles in the Rapidly-Rotating Young Solar Analog HD 30495
• Structure of prominence legs: Plasma and magnetic field
• A closer look at a coronal loop rooted in a sunspot umbra
• On the Active Region Bright Grains Observed in the Transition Region Imaging Channels of IRIS
• Multi-scale observations of thermal non-equilibrium cycles in coronal loops
• Transition Region and Chromospheric Signatures of Impulsive Heating Events. II. Modeling
• IRIS, Hinode, SDO, and RHESSI observations of a white light flare produced directly by non-thermal electrons
• Investigating the Transition Region Explosive Events and Their Relationship to Network Jets
• Study on Precursor Activity of the X1.6 Flare in the Great AR 12192 with SDO, IRIS, and Hinode
• Self-absorption in the solar transition region
• Doppler shift oscillations from a hot line observed by IRIS
• Observations of the Kelvin-Helmholtz instability driven by dynamic motions in a solar prominence
• Signatures of ubiquitous magnetic reconnection in the lower solar atmosphere
• Onset of turbulent fast magnetic reconnection observed in the solar atmosphere
• A Two-ribbon White-light Flare Associated with a Failed Solar Eruption Observed by ONSET, SDO, and IRIS
• On the Misalignment between Chromospheric Features and the Magnetic Field on the Sun
• The solar chromosphere at millimetre and ultraviolet wavelengths. I. Radiation temperatures and a detailed comparison
• Different Signatures of Chromospheric Evaporation in Two Solar Flares Observed with IRIS
• Observation of a reversal of breakout reconnection preceding a jet: evidence of oscillatory magnetic reconnection?
• Temperature constraints from inversions of synthetic solar optical, UV and radio spectra
• Observations and modeling of the onset of fast reconnection in the solar transition region
• Ambipolar diffusion in the Bifrost code
• Hinode and IRIS observations of the magnetohydrodynamic waves propagating from the photosphere to the chromosphere in a sunspot
• On the multi-threaded nature of solar spicules
• Explosive chromospheric evaporation driven by nonthermal electrons around one footpoint of a solar flare loop
• Spectral Evidence for Heating at Large Column Mass in Umbral Solar Flare Kernels I: IRIS NUV Spectra of the X1 Solar Flare of 2014 Oct 25
• First simultaneous SST/CRISP and IRIS observations of a small-scale quiet Sun vortex
• The Frequency-dependent Damping of Slow Magnetoacoustic Waves in a Sunspot Umbral Atmosphere
• Observations and Modelling of the Pre-Flare Period of the 29 March 2014 X1 Flare
• Chromospheric heating due to cancellation of quiet Sun internetwork fields
• Spectroscopic Signatures Related to a Sunquake
• Time Dependent Non-Equilibrium Ionization of Transition Region Lines Observed with IRIS
• Simulations of prominence eruption preceded with large amplitude longitudinal oscillations and draining
• Observationally based models of penumbral microjets
• Mg II Lines Observed during the X-class Flare on 29 March 2014 by the Interface Region Imaging Spectrograph
• Solar Flare Arcade Modelling: Bridging the gap from 1D to 3D Simulations of Optically Thin Radiation
• Reconstruction of a helical prominence in 3D from IRIS spectra and images
• Multi-layered Kelvin-Helmholtz Instability in the Solar Corona
• A Si IV/O IV electron density diagnostic for the analysis of IRIS solar spectra
• IRIS observations of magnetic interactions in the solar atmosphere between pre-existing and emerging magnetic fields. II. UV emission properties
• The Statistical Relationship between White-light Emission and Photospheric Magnetic Field Changes in Flares
• First High-resolution Spectroscopic Observations of an Erupting Prominence Within a Coronal Mass Ejection by the Interface Region Imaging Spectrograph (IRIS)
• Dynamics in Sunspot Umbra as Seen in New Solar Telescope and Interface Region Imaging Spectrograph Data
• Magnetic braids in eruptions of a spiral structure in the solar atmosphere
• Automated Swirl Detection Algorithm (ASDA) and Its Application to Simulation and Observational Data
• Imaging and spectral study on the null point of a fan-spine structure during a solar flare
• Helical motions of fine-structure prominence threads observed by Hinode and IRIS
• Differences between Doppler velocities of ions and neutral atoms in a solar prominence
• Coronal Mini-jets in an Activated Solar Tornado-like Prominence
• Electron Beams Cannot Directly Produce Coronal Rain
• ALMA detection of dark chromospheric holes in the quiet Sun
• Spectroscopic Observations of Magnetic Reconnection and Chromospheric Evaporation in an X-shaped Solar Flare
• Formation and Eruption of a Small Flux Rope in the Chromosphere Observed by NST, IRIS, and SDO
• Modelling Mg II During Solar Flares. I. Partial Frequency Redistribution, Opacity, and Coronal Irradiation
• Tracing the Chromospheric and Coronal Magnetic Field with AIA, IRIS, IBIS, and ROSA Data
• Observations of Transient Active Region Heating with Hinode
• Properties and Modeling of Unresolved Fine Structure Loops Observed in the Solar Transition Region by IRIS
• On Magnetic Activity Band Overlap, Interaction, and the Formation of Complex Solar Active Regions
• IRIS Si IV Line Profiles at Flare Ribbons as Indications of Chromospheric Condensation
• A White-light Flare Powered by Magnetic Reconnection in the Lower Solar Atmosphere
• A Steady-state Supersonic Downflow in the Transition Region above a Sunspot Umbra
• Light Walls Around Sunspots Observed by the Interface Region Imaging Spectrograph
• Joint X-ray, EUV and UV Observations of a Small Microflare
• Thermal responses in a coronal loop maintained by wave heating mechanisms
• Spectroscopic and Stereoscopic Observations of the Solar Jets
• Diagnosing transient ionization in dynamic events
• A persistent quiet-Sun small-scale tornado III. Waves
• Bridging the Gap: Capturing the Ly$\alpha$ Counterpart of a Type-II Spicule and its Heating Evolution with VAULT2.0 and IRIS Observations
• Chromospheric and Coronal Wave Generation in a Magnetic Flux Sheath
• The Formation Height of Millimeter-wavelength Emission in the Solar Chromosphere
• Emission of solar chromospheric and transition region features related to the underlying magnetic field
• Automated Spatiotemporal Analysis of Fibrils and Coronal Rain using the Rolling Hough Transform
• On the origin of the magnetic energy in the quiet solar chromosphere
• Simulations of Alfven wave driving of the solar chromosphere - efficient heating and spicule launching
• Efficient Calculation of Non-Local Thermodynamic Equilibrium Effects in Multithreaded Hydrodynamic Simulations of Solar Flares
• Narrow-line-width UV bursts in the transition region above Sunspots observed by IRIS
• Emergence of granular-sized magnetic bubbles through the solar atmosphere. III. The path to the transition region
• High-frequency spicule oscillations generated via mode conversion
• On the importance of the nonequilibrium ionization of Si IV and O IV and the line-of-sight in solar surges
• On the origin of the flare emission in IRIS' SJI 2832 filter: Balmer continuum or spectral lines?
• The role of small-scale surface motions in the transfer of twist to a solar jet from a remote stable flux rope
• IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules in a Solar Polar Coronal Hole
• Magnetic Energy Dissipation during the 2014 March 29 Solar Flares
• ALMA Observations of the Solar Chromosphere on the Polar Limb
• On the relation between transition region network jets and coronal plumes
• Modelling of Mg II lines in solar prominences
• Estimating the temperature and density of a spicule from 100 GHz data obtained with ALMA
• Quiet-Sun and Coronal Hole in \ion{Mg}{2}~k line as observed by IRIS
• Signatures of magnetic reconnection at the footpoints of fan shape jets on a light bridge driven by photospheric convective motions
• Impulsive coronal heating from large-scale magnetic rearrangements: from IRIS to SDO/AIA
• ALMA and IRIS Observations of the Solar Chromosphere I: an On-Disk Type II Spicule
• A solar flare disturbing a light wall above a sunspot light bridge
• Observational Evidence of Magnetic Reconnection Associated with Magnetic Flux Cancellation
• Formation of coronal rain triggered by impulsive heating associated with magnetic reconnection
• The Multi-Species Farley-Buneman Instability in the Solar Chromosphere
• Two Solar Tornadoes Observed with the Interface Region Imaging Spectrograph
• Oscillatory Response of the Solar Chromosphere to a Strong Downflow above a Sunspot
• ALMA and IRIS Observations of the Solar Chromosphere II: Structure and Dynamics of Chromospheric Plage
• Evidence for the two fluid scenario in solar prominences
• Three-dimensional Magnetic Reconnection Triggering an X-class Confined Flare in Active Region 12192
• IRIS observations of the low-atmosphere counterparts of active region outflows
• The Triggering of the 29-March-2014 Filament Eruption
• Relation of coronal rain originating from coronal condensations to interchange magnetic reconnection
• Multi-wavelength Study of Transition Region Penumbral Subarcsecond Bright Dots Using IRIS and NST
• High-resolution Observations of a Flux Rope with the Interface Region Imaging Spectrograph
• The Formation of IRIS Diagnostics. IX. The Formation of the C I 135.58 Line in the Solar Atmosphere
• Relationship between chromospheric evaporation and magnetic field topology in M-class solar flare
• Statistical Investigation of Supersonic Downflows in the Transition Region above Sunspots
• Resonant absorption: transformation of compressive motions into vortical motions
• Observations of an X-shaped Ribbon Flare in the Sun and Its Three-dimensional Magnetic Reconnection
• Modeling a Propagating Sawtooth Flare Ribbon Structure as a Tearing Mode in the Presence of Velocity Shear
• Simulating Solar Flare Irradiance with Multithreaded Models of Flare Arcades
• Non-thermal line broadening due to braiding-induced turbulence in solar coronal loops
• Untwisting Jets Related to Magnetic Flux Cancellation
• Signatures of ubiquitous magnetic reconnection in the deep atmosphere of sunspot penumbrae
• Statistical Study of Chromospheric Evaporation in Impulsive Phase of Solar Flares
• Observations of upward propagating waves in the transition region and corona above Sunspots
• Average radial structures of gas convection in the solar granulation
• On the spectroscopic detection of periodic plasma flows in loops undergoing thermal non-equilibrium
• Plasma injection into a solar coronal loop
• Subarcsecond Bright Points and Quasi-periodic Upflows Below a Quiescent Filament Observed by the IRIS
• Spectroscopic Diagnostics of Solar Magnetic Flux Ropes Using Iron Forbidden Line
• Quantifying the Influence of Key Physical Processes on the Formation of Emission Lines Observed by IRIS: I. Non-Equilibrium Ionization and Density-Dependent Rates
• Temporal and Spatial Scales in Coronal Rain Revealed by UV Imaging and Spectroscopic Observations
• Transition region loops in the very late phase of flux-emergence in IRIS sit-and-stare observations
• Non-equilibrium ionization by a periodic electron beam II. Synthetic Si IV and O IV transition region spectra
• Synthetic Emissions of the Fe XXI 1354 Å Line from Flare Loops Experiencing Fundamental Fast Sausage Oscillations
• Kelvin-Helmholtz instability and Alfvenic vortex shedding in solar eruptions
• Penumbral micro-jets at high spatial and temporal resolution
• What Is the Source of Quiet Sun Transition Region Emission?
• Chromospheric peculiar off-limb dynamical events from IRIS observations
• Continuum enhancements, line profiles and magnetic field evolution during consecutive flares
• The dark side of penumbral microjets: Observations in Hα
• Evolution Of Downflows In The Transition Region Above A Sunspot Over Short Time-Scales
• A multi-diagnostic spectral analysis of penumbral microjets
• Chromospheric UV bursts and turbulent driven magnetic reconnection
• A persistent quiet-Sun small-scale tornado. II. Oscillations
• Fine structure above a light bridge in the transition region and corona

Cited by in corpus (1)

• Solar jets observed with the Interface Region Imaging Spectrograph (IRIS)