The Solar Optical Telescope for the Hinode Mission: An Overview

Abstract

The Solar Optical Telescope (SOT) aboard the Hinode satellite (formerly called Solar-B) consists of the Optical Telescope Assembly (OTA) and the Focal Plane Package (FPP). The OTA is a 50 cm diffraction-limited Gregorian telescope, and the FPP includes the narrow-band (NFI) and wide-band (BFI) filtergraphs, plus the Stokes spectro-polarimeter (SP). SOT provides unprecedented high resolution photometric and vector magnetic images of the photosphere and chromosphere with a very stable point spread function, and is equipped with an image stabilization system that reduces the error to less than 0.01 arcsec rms. Together with the other two instruments on Hinode (the X-Ray Telescope (XRT) and EUV Imaging Spectrometer (EIS)), SOT is poised to address many fundamental questions about solar magneto-hydrodynamics. Note that this is an overview, and the details of the instrument are presented in a series of companion papers.

References in corpus (4)

• An Ab Initio Approach to the Solar Coronal Heating Problem
• The solar magnetic field
• Dynamic Fibrils are driven by Magnetoacoustic Shocks
• Magnetic flux emergence in granular convection: Radiative MHD simulations and observational signatures

Cited by in corpus (637)

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• Simulations of stellar convection with CO5BOLD
• Evolution of Magnetic Field and Energy in A Major Eruptive Active Region Based on SDO/HMI Observation
• A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
• VFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magnetic Imager
• Observing the Roots of Solar Coronal Heating - in the Chromosphere
• Simulation of the Formation of a Solar Active Region
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• Solar UV and X-Ray Spectral Diagnostics
• The Polarimetric and Helioseismic Imager on Solar Orbiter
• Magnetic Landscape of Sun's Polar Region
• Magnetic Field Structures Triggering Solar Flares and Coronal Mass Ejections
• Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
• On-disk counterparts of type II spicules in the Ca II 854.2 nm and Halpha lines
• On the generation of solar spicules and Alfvénic waves
• Quantifying Spicules
• Propagating waves along spicules
• The Magnetic Field in the Solar Atmosphere
• Giant Chromospheric Anemone Jet Observed with Hinode and Comparison with Magnetohydrodynamic Simulations: Evidence of Propagating Alfven Waves and Magnetic Reconnection
• Solar surface emerging flux regions: a comparative study of radiative MHD modeling and Hinode SOT observations
• Alfven Waves in the Solar Atmosphere
• Response of the Photospheric Magnetic Field to the X2.2 Flare on 2011 February 15
• Magnetic Flux Transport at the Solar Surface
• Magnetic Structure of Sunspots
• Small-scale solar magnetic fields
• Emergence of small-scale magnetic loops through the quiet solar atmosphere
• Solar science with the Atacama Large Millimeter/submillimeter Array - A new view of our Sun
• Coronal rain as a marker for coronal heating mechanisms
• The intensity contrast of solar granulation: comparing Hinode SP results with MHD simulations
• The second flight of the SUNRISE balloon-borne solar observatory: overview of instrument updates, the flight, the data and first results
• Spatially coupled inversion of spectro-polarimetric image data I: Method and first results
• Properties of Magneto-Hydrodynamic Waves in the Solar Photosphere with Hinode
• Nonlinear propagation of Alfven waves driven by observed photospheric motions: Application to the coronal heating and spicule formation
• Solar Force-free Magnetic Fields
• Observation of kink instability during small B5.0 solar flare on 04 June, 2007
• Large Amplitude Oscillations in Prominences
• Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. I- Observational aspects
• Physical Properties of a Sunspot Chromosphere with Umbral Flashes
• Signatures of Alfven waves in the polar coronal holes as seen by EIS/Hinode
• Probing quiet Sun magnetism using MURaM simulations and Hinode/SP results: support for a local dynamo
• The multi-thermal and multi-stranded nature of coronal rain
• Quiet Sun magnetic fields observed by Hinode: Support for a local dynamo
• High-resolution observations of flare precursors in the low solar atmosphere
• Homologous Helical Jets: Observations by IRIS, SDO and Hinode and Magnetic Modeling with Data-Driven Simulations
• Multiwavelength Observations of Small-Scale Reconnection Events triggered by Magnetic Flux Emergence in the Solar Atmosphere
• The Solar Internetwork. I. Contribution to the Network Magnetic Flux
• Peripheral downflows in sunspot penumbrae
• Solar magnetic fields as revealed by Stokes polarimetry
• An Intriguing Chromospheric Jet Observed by Hinode: I. Fine Structure Kinematics and Evidence of Unwinding Twists
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• Observation and Simulation of Longitudinal Oscillations of an Active Region Prominence
• Rapid Changes of Photospheric Magnetic Field after Tether-Cutting Reconnection and Magnetic Implosion
• Polar Field Reversal Observations with Hinode
• Ubiquitous High Speed Transition Region and Coronal Upflows in the Quiet Sun
• Comparison of transient horizontal magnetic fields in a plage region and in the quiet Sun
• Chromospheric Jet and Growing "Loop" Observed by Hinode: New Evidence of Fan-Spine Magnetic Topology Resulting From Flux Emergence
• On-Orbit Degradation of Solar Instruments
• Structure of sunspot penumbral filaments: a remarkable uniformity of properties
• On the Role of Rotating Sunspots in the Activity of Solar Active Region NOAA 11158
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• Point spread functions for the Solar Optical Telescope onboard Hinode
• Is the Polar Region Different from the Quiet Region of the Sun?
• Observing Episodic Coronal Heating Events Rooted in Chromospheric Activity
• The Influence of Spatial Resolution on Nonlinear Force-Free Modeling
• Estimating the "Dark" Energy Content of the Solar Corona
• On the 2012 October 23 circular ribbon flare: emission features and magnetic topology
• Prominence Formation Associated with an Emerging Helical Flux Rope
• Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
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• Magnetic Energy and Helicity Budgets in the Active-Region Solar Corona. II. Nonlinear Force-Free Approximation
• The discovery of geomagnetically trapped cosmic ray antiprotons
• Light Bridge in a Developing Active Region. I. Observation of Light Bridge and its Dynamic Activity Phenomena
• Coronal hole boundaries at small scales: IV. SOT view Magnetic field properties of small-scale transient brightenings in coronal holes
• Transverse oscillations of loops with coronal rain observed by Hinode/SOT
• Revision of Solar Spicule Classification
• Turbulent magnetic fields in the quiet Sun: implications of Hinode observations and small-scale dynamo simulations
• Structure and Dynamics of Isolated Internetwork Ca II H Bright Points Observed by Sunrise
• X-ray and EUV Observations of Simultaneous Short and Long Period Oscillations in Hot Coronal Arcade Loops
• Spicule-like structures observed in 3D realistic MHD simulations
• How to Train Your Flare Prediction Model: Revisiting Robust Sampling of Rare Events
• Inferring the magnetic field vector in the quiet Sun. I. Photon noise and Selection Criteria
• Waves in the lower solar atmosphere: the dawn of next-generation solar telescopes
• A Non-radial Eruption in a Quadrupolar Magnetic Configuration with a Coronal Null
• Chromospheric Condensation and Quasi-periodic Pulsations in a Circular-ribbon Flare
• On the continuum intensity distribution of the solar photosphere
• Microwave Quasi-periodic Pulsations in Multi-timescales Associated with a Solar Flare/CME Event
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• Nonlinear Force-Free Extrapolation of the Coronal Magnetic Field Based on the MHD Relaxation Method
• Enhancing SDO/HMI images using deep learning
• Magnetohydrodynamic Simulation of the X2.2 Solar Flare on 2011 February 15: II. Dynamics Connecting the Solar Flare and the Coronal Mass Ejection
• Numerical Simulations of Solar Chromospheric Jets Associated with Emerging Flux
• The solar chromosphere at high resolution with IBIS: III. Comparison of Ca II K and Ca II 854.2 nm imaging
• Transverse Wave Induced Kelvin-Helmholtz Rolls in Spicules
• Mapping Solar Magnetic Fields from the Photosphere to the Base of the Corona
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• Statistical Distribution of Size and Lifetime of Bright Points Observed with the New Solar Telescope
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• The Instruments and Capabilities of the Miniature X-ray Solar Spectrometer (MinXSS) CubeSats
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• Observations and numerical models of solar coronal heating associated with spicules
• Numerical Simulations of the Magnetic Rayleigh-Taylor Instability in the Kippenhahn-Schlüter Prominence Model
• Hemispheric Helicity Trend for Solar Cycle 24
• Evolution of Currents of Opposite Signs in the Flare Productive Solar Active Region NOAA 10930
• A geometrical height scale for sunspot penumbrae
• On the velocity field of sunspot penumbrae - I. A global view
• Supersonic Downflows in a Sunspot Light Bridge
• Buildup and Release of Magnetic Twist during the X3.4 Solar Flare of December 13, 2006
• The continuum intensity as a function of magnetic field I. Active region and quiet Sun magnetic elements
• Intermittency Spectra of the Magnetic Field in Solar Active Regions
• Impact of Type II Spicules in the Corona: Simulations and Synthetic Observables
• Study of Two Successive Three-Ribbon Solar Flares on 2012 July 6
• Small-scale chromospheric jets above a sunspot light bridge
• Depth-dependent global properties of a sunspot observed by Hinode using the Solar Optical Telescope/Spectropolarimeter
• 3-D non-LTE radiative transfer effects in Fe I lines: II. Line formation in 3-D radiation hydrodynamic simulations
• Horizontal flow fields observed in Hinode G-band images. I. Methods
• Different Patterns of Chromospheric Evaporation in a Flaring Region Observed with Hinode/EIS
• Dynamics of the solar atmosphere above a pore with a light bridge
• Precursor of Sunspot Penumbral Formation discovered with Hinode SOT Observations
• Can coronal hole spicules reach coronal temperatures?
• Detection of the strongest magnetic field in a sunspot light bridge
• Velocity and Magnetic Transients Driven by the X2.2 White-Light Flare of 2011 February 15 in NOAA 11158
• Record-breaking coronal magnetic field in solar active region 12673
• The frontier between Small-scale bipoles and Ephemeral Regions in the solar photosphere: Emergence and Decay of an Intermediate-scale bipole observed with IMaX/SUNRISE
• Various Local Heating Events in the Earliest Phase of Flux Emergence
• 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
• Detection of Small-Scale Granular Structures in the Quiet Sun with the New Solar Telescope
• The Solar Internetwork. II. Magnetic Flux Appearance and Disappearance Rates
• Magnetic Flux Emergence and Decay Rates for Preceder and Follower Sunspots Observed with HMI
• The causality between the rapid rotation of a sunspot and an X3.4 flare
• Evidence for a Transition Region response to penumbral microjets in sunspots
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• Time Evolution of Coronal Magnetic Helicity in the Flaring Active Region NOAA 10930
• Parameters of the Magnetic Flux inside Coronal Holes
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• The magnetic nature of umbra-penumbra boundary in sunspots
• Magnetic field strength distribution of magnetic bright points inferred from filtergrams and spectro-polarimetric data
• On the propagation of p-modes into the solar chromosphere
• IRIS observations of magnetic interactions in the solar atmosphere between pre-existing and emerging magnetic fields. I. Overall evolution
• Rayleigh-Taylor instability in partially ionized compressible plasmas: one fluid approach
• Horizontal flow fields observed in Hinode G-band images II. Flow fields in the final stages of sunspot decay
• Strongly Blueshifted Phenomena Observed with {\it Hinode}/EIS in the 2006 December 13 Solar Flare
• Evidence of Explosive Evaporation in a Microflare Observed by Hinode/EIS
• Photospheric magnetic structure of coronal holes
• A Magnetic Calibration of Photospheric Doppler Velocities
• A Statistical Analysis of the SOT-Hinode Observations of Solar Spicules and their Wave-like Behavior
• Spectropolarimetric inversions of the Ca ii 8542 Å line in a M-class solar flare
• Diffusion of solar magnetic elements up to supergranular spatial and temporal scales
• Fast Solar Image Classification Using Deep Learning and its Importance for Automation in Solar Physics
• On Kelvin-Helmholtz and parametric instabilities driven by coronal waves
• On the solar chromosphere observed at the limb with Hinode
• The Role of Partial Ionization Effects in the Chromosphere
• Persistent magnetic vortex flow at a supergranular vertex
• Effect of Polarimetric Noise on the Estimation of Twist and Magnetic Energy of Force-Free Fields
• A new type of small-scale downflow patches in sunspot penumbrae
• Achieving Self-Consistent Nonlinear Force-free Modeling of Solar Active Regions
• Is the sky the limit? Performance of the revamped Swedish 1-m Solar Telescope and its blue- and red-beam re-imaging systems
• Magnetic Flux Loss and Flux Transport in a Decaying Active Region
• Interpretation of HINODE SOT/SP asymmetric Stokes profiles observed in quiet Sun network and internetwork
• A High-Resolution Three-Dimensional Model of the Solar Photosphere Derived from Hinode Observations
• Magnetic field in atypical prominence structures: Bubble, tornado and eruption
• Explosive events - swirling transition region jets
• Direct Imaging of Fine Structure in the Chromosphere of a Sunspot Umbra
• Observations of Chromospheric Anemone Jets with Hinode SOT and Hida Ca II Spectroheliogram
• On the Absence of Photospheric Net Currents in Vector Magnetograms of Sunspots Obtained From Hinode (SOT/SP)
• Structure of prominence legs: Plasma and magnetic field
• Three-dimensional non-LTE radiative transfer effects in Fe I lines I. Flux sheet and flux tube geometries
• Scaling laws for magnetic fields on the quiet Sun
• Characteristic Dependence of Umbral Dots on their Magnetic Structure
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• Statistical Study on the Nature of Solar Flux Emergence
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• Granular-Scale Elementary Flux Emergence Episodes in a Solar Active Region
• Spatial deconvolution of spectropolarimetric data: an application to quiet Sun magnetic elements
• Large-amplitude longitudinal oscillations in a solar filament
• Two-step Emergence of the Magnetic Flux Sheet from the Solar Convection Zone
• Structure and Stability of Magnetic Fields in Solar Active Region12192 Based on Nonlinear Force-Free Field Modeling
• The Photospheric Poynting Flux and Coronal Heating
• Study of single-lobed circular polarization profiles in the quiet Sun
• Vertical flows and mass flux balance of sunspot umbral dots
• The Effects of Spatio-temporal Resolution on Deduced Spicule Properties
• Local Helioseismology of Sunspots: Current Status and Perspectives (Invited Review)
• Propagation of sausage soliton in the solar lower atmosphere observed by Hinode/SOT
• Hinode and IRIS observations of the magnetohydrodynamic waves propagating from the photosphere to the chromosphere in a sunspot
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• On the multi-threaded nature of solar spicules
• The solar chromosphere observed at 1 Hz and 0."2 resolution
• Plasma Beta Stratification in the Solar Atmosphere: A Possible Explanation for the Penumbra Formation
• Pervasive Linear Polarization Signals in the Quiet Sun
• Observationally based models of penumbral microjets
• Horizontal or vertical magnetic fields on the quiet Sun: Angular distributions and their height variations
• Chromospheric heating due to cancellation of quiet Sun internetwork fields
• Chromospheric polarimetry through multi-line observations of the 850 nm spectral region
• Solar surface and atmospheric dynamics: The Photosphere
• Probing deep photospheric layers of the quiet Sun with high magnetic sensitivity
• Sunrise III: Overview of Observatory and Instruments
• HINODE Observations of Chromospheric Brightenings in the Ca II H Line during small-scale Flux Emergence Events
• Optimization of Photospheric Electric Field Estimates for Accurate Retrieval of Total Magnetic Energy Injection
• Plasmoids, Flows, and Jets During Magnetic Reconnection in a Failed Solar Eruption
• A distinct magnetic property of the inner penumbral boundary
• Quiet-Sun imaging asymmetries in NaI D1 compared with other strong Fraunhofer lines
• Spatial and temporal distributions of transient horizontal magnetic fields with deep exposure
• Advances in Global and Local Helioseismology: an Introductory Review
• Radiative emission of solar features in the Ca II K line: comparison of measurements and models
• Intensity contrast from MHD simulations and from HINODE observations
• A distinct magnetic property of the inner penumbral boundary. II. Formation of a penumbra at the expense of a pore
• Characterization of horizontal flows around solar pores from high-resolution time series of images
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• Characteristics that Produce White-Light Enhancements in Solar Flares Observed by Hinode/SOT
• Propagating Spectropolarimetric Disturbances in a Large Sunspot
• On the Force-Freeness of the Photospheric Sunspot Magnetic Fields as Observed from Hinode (SOT/SP)
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• A comparison of preprocessing methods for solar force-free magnetic field extrapolation
• Ubiquitous quiet-Sun jets
• Reconstruction of a helical prominence in 3D from IRIS spectra and images
• Lagrangian coherent structures in photospheric flows and their implications for coronal magnetic structure
• On the Collective Magnetic Field Strength and Vector Structure of Dark Umbral Cores Measured by the Hinode Spectropolarimeter
• Imaging and spectral study on the null point of a fan-spine structure during a solar flare
• Automated Swirl Detection Algorithm (ASDA) and Its Application to Simulation and Observational Data
• Magnetohydrodynamic Simulations for Studying Solar Flare Trigger Mechanism
• MHD wave modes resolved in fine-scale chromospheric magnetic structures
• Analysis of a Fragmenting Sunspot using Hinode Observations
• Helical motions of fine-structure prominence threads observed by Hinode and IRIS
• A new MHD-assisted Stokes inversion technique
• Multiwavelength Study of M8.9/3B Solar Flare from AR NOAA 10960
• Testing the Accuracy of Data Driven MHD Simulations of Active Region Evolution
• Triggering Process of the X1.0 Three-ribbon Flare in the Great Active Region NOAA 12192
• Dual Trigger of Transverse Oscillations in a Prominence by EUV Fast and Slow Coronal Waves: SDO/AIA and STEREO/EUVI Observations
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• Understanding the white-light flare on 2012 March 9 : Evidence of a two-step magnetic reconnection
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• Comparison of Nonlinear Force-free Field and Potential Field in the Quiet Sun
• Unusual Filaments Inside the Umbra
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• A rising cool column as signature for helical flux emergence and formation of prominence and coronal cavity
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• Solar source of energetic particles in interplanetary space during the 2006 December 13 event
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• Modelling and Interpreting The Effects of Spatial Resolution on Solar Magnetic Field Maps
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• Statistical Relation between Solar Flares and Coronal Mass Ejections with Respect to Sigmoidal Structures in Active Regions
• Flares and rotation of M dwarfs with habitable zones accessible to TESS planet detections
• Non-LTE inversions of a confined X2.2 flare: I. Vector magnetic field in the photosphere and chromosphere
• Bridging the Gap: Capturing the Ly$\alpha$ Counterpart of a Type-II Spicule and its Heating Evolution with VAULT2.0 and IRIS Observations
• The continuum intensity as a function of magnetic field II. Local magnetic flux and convective flows
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• Magnetic Flux Rope Shredding by a Hyperbolic Flux Tube: The Detrimental Effects of Magnetic Topology on Solar Eruptions
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• The potential of many-line inversions of photospheric spectropolarimetric data in the visible and near UV
• Evolution of the Kippenhahn-Schlueter Prominence Model Magnetic Field Under Cowling Resistivity
• Understanding the HMI pseudocontinuum in white-light solar flares
• Solar Ultraviolet Bursts in a Coordinated Observation of IRIS, Hinode and SDO
• Dynamics of subarcsecond bright dots in the transition region above sunspot and their relation to penumbral micro-jets
• The problem of the height dependence of magnetic fields in sunspots
• Reconnection Electric Field and Hardness of X-Ray Emission of Solar Flares
• Vertical magnetic field gradient in the photospheric layers of sunspots
• Chromospheric Plasma Ejections in a Light Bridge of a Sunspot
• The properties of horizontal magnetic elements in quiet solar intranetwork
• Analysis of Flows Inside Quiescent Prominences as Captured by Hinode/Solar Optical Telescope
• The free energy of NOAA active region AR 11029
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• IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules in a Solar Polar Coronal Hole
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• Comparison between Hinode/SOT and SDO/HMI, AIA Data for the Study of the Solar Flare Trigger Process
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• Magnetic helicity estimations in models and observations of the solar magnetic field. Part IV: Application to solar observations
• Explanation of the sea-serpent magnetic structure of sunspot penumbrae
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• Co-spatial velocity and magnetic swirls in the simulated solar photosphere
• Increasing the Fine Structure Visibility of the Hinode SOT Ca II H Filtergrams
• High-resolution imaging and near-infrared spectroscopy of penumbral decay
• The coronal energy input from magnetic braiding
• The Association of Polar Faculae with Polar Magnetic Patches Examined with Hinode Observations
• Development of a Precise Polarization Modulator for UV Spectropolarimetry
• Evolution of twist-shear and dip-shear during X-class flare of 13 December 2006: Hinode observations
• Nature of Quiet Sun Oscillations Using Data from the Hinode, TRACE, and SOHO Spacecraft
• Combining magneto-hydrostatic constraints with Stokes profile inversions. II. Application to Hinode/SP observations
• Three-dimensional magnetic structure of a sunspot: comparison of the photosphere and upper chromosphere
• Multi-wavelength spectroscopic observation of EUV jet in AR 10960
• On spectropolarimetric measurements with visible lines
• Imaging Spectropolarimeter for Multi-application Solar Telescope at Udaipur Solar Observatory: Characterization of polarimeter and preliminary observations
• On the flare induced seismicity in the active region NOAA 10930 and related enhancement of global waves in the sun
• The Triggering of the 29-March-2014 Filament Eruption
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• High-Cadence Imaging and Imaging Spectroscopy at the GREGOR Solar Telescope - A Collaborative Research Environment for High-Resolution Solar Physics
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• The small-scale structure of photospheric convection retrieved by a deconvolution technique applied to Hinode/SP data
• Coronal loops above an Active Region - observation versus model
• Non-magnetic photospheric bright points in 3D simulations of the solar atmosphere
• On the Performance of Multi-Instrument Solar Flare Observations During Solar Cycle 24
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• Disintegration of Magnetic Flux in Decaying Sunspots as Observed with the Hinode SOT
• Magnetic helicity transported by flux emergence and shuffling motions in Solar Active Region NOAA 10930
• Slipping reconnection in a solar flare observed in high resolution with the GREGOR solar telescope
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• Properties of the Umbral Filament Observed in Active Region NOAA 12529
• Formal Solutions for Polarized Radiative Transfer. IV. Numerical Performances in Practical Problems
• Analysis of a spatially deconvolved solar pore
• Evolution of small-scale magnetic elements in the vicinity of granular-size swirl convective motions
• Orphan penumbrae: Submerging horizontal fields
• Emergence of small-scale magnetic flux in the quiet Sun
• Relationship between supergranulation flows, magnetic cancellation and network flares
• Comment on "Resolving the 180-deg Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions"
• Chromospheric observations and magnetic configuration of a supergranular structure
• Fast Inversion of Solar Ca II Spectra in Non-Local Thermodynamic Equilibrium
• Doubts about the crucial role of the rising-tube mechanism in the formation of sunspot groups
• A distinct magnetic property of the inner penumbral boundary III. Analysis of simulated sunspots
• In-situ generation of transverse MHD waves from colliding flows in the solar corona
• Transport of magnetic flux from the canopy to the internetwork
• Observations of solar small-scale magnetic flux-sheet emergence
• On Identifying and Mitigating Bias in Inferred Measurements for Solar Vector Magnetic Field Data
• A Laboratory Experiment of Magnetic Reconnection: Outflows, Heating and Waves in Chromospheric Jets
• Chromospheric signatures of small-scale flux emergence as observed with NST and Hinode instruments
• Variations of the 3-D coronal magnetic field associated with the X3.4-class solar flare event of AR 10930
• The formation of an atypical sunspot light bridge as a result of large-scale flux emergence
• The Solar Oxygen Abundance from an Empirical Three-Dimensional Model
• Plasma properties and Stokes profiles during the lifetime of a photospheric magnetic bright point
• Cancellation of Small-Scale Magnetic Features
• Multi-Wavelength Observation of Electron Acceleration in the 2006 December 13 Flare
• Comparing UV/EUV line parameters and magnetic field in a quiescent prominence with tornadoes
• Centre-to-limb spectro-polarimetric diagnostics of simulated solar photospheric magneto-convection: signatures of photospheric Alfven waves
• What is the true nature of blinkers?
• Supersonic Downflows at the Umbra-Penumbra Boundary of Sunspots
• Observational evidence for two-component distributions describing solar magnetic bright points
• Investigating prominence turbulence with Hinode SOT Dopplergrams
• Super-diffusion versus competitive advection: a simulation
• Classification of High-resolution Solar Hα Spectra using t-distributed Stochastic Neighbor Embedding
• Chromospheric magnetic field: A comparison of He I 10830 A observations with nonlinear force-free field extrapolation
• The Trigger Mechanism of Recurrent Solar Active Region Jets Revealed by the Magnetic Properties of a Coronal Geyser Site
• Magnetic Helicity Reversal in the Corona at Small Plasma Beta
• Chromospheric Magnetic Reconnection caused by Photospheric Flux Emergence: Implications for Jet-like Events Formation
• The dark side of solar photospheric G-band bright points
• High-resolution imaging spectroscopy of two micro-pores and an arch filament system in a small emerging-flux region
• Magnetic Tension of Sunspot Fine Structures
• Response of SDO/HMI observables to heating of the solar atmosphere by precipitating high-energy electrons
• High speed magnetized flows in the quiet Sun
• Magnetic Non-Potentiality of Solar Active Regions and Peak X-Ray Flux of the Associated Flares
• Average radial structures of gas convection in the solar granulation
• Temporal relation between quiet-Sun transverse fields and the strong flows detected by IMaX/SUNRISE
• Simulation of a flux emergence event and comparison with observations by Hinode
• Evolution of the critical torus instability height and CME likelihood in solar active regions
• Transport of internetwork magnetic flux elements in the solar photosphere
• Response to "Comment on `Resolving the 180deg Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions'"
• Occurrence and persistence of magnetic elements in the quiet Sun
• Ultra-high-resolution Observations of MHD Waves in Photospheric Magnetic Structures
• Milne-Eddington inversion of the Fe I line pair at 630~nm
• Intrusion of Magnetic Peninsula toward the Neighboring Opposite-polarity Region That Triggers the Largest Solar Flare in Solar Cycle 24
• Inference of electric currents in the solar photosphere
• Kinematics and Magnetic Properties of a Light Bridge in a Decaying Sunspot
• Penumbral decay observed in active region NOAA 12585
• 3D magnetic field configuration of small-scale reconnection events in the solar plasma atmosphere
• IBIS-A: The IBIS data Archive. High resolution observations of the solar photosphere and chromosphere with contextual data
• Analysis of spatially deconvolved polar faculae
• The Evershed Effect with SOT/Hinode
• Observations of Umbral Dots and their Physical Models
• Critical magnetic field strengths for solar coronal plumes in quiet regions and coronal holes?
• Unresolved Mixed Polarity Magnetic Fields at Flux Cancellation Site in Solar Photosphere at 0".3 Spatial Resolution
• On the Area Expansion of Magnetic Flux-Tubes in Solar Active Regions
• Resolving Azimuth Ambiguity Using Vertical Nature of Solar Quiet-Sun Magnetic Fields
• Rapid Enhancement of Sheared Evershed Flow Along the Neutral Line Associated with an X6.5 Flare Observed by Hinode
• Magnetic topology of a naked sunspot: Is it really naked?
• Magnetic properties on the boundary of an evolving pore
• On the origin of reverse polarity patches found by Hinode in sunspot penumbrae
• The Evolution of Sunspot Magnetic Fields Associated with a Solar Flare
• The solar internetwork. III. Unipolar versus bipolar flux appearance
• Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar disk
• Long-term trends of magnetic bright points: I. Number of MBPs at disc centre
• Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage
• Flare Energy Release in the Magnetic Field Polarity Inversion Line During M1.2 Solar Flare of March 15, 2015. Paper I. Onset of Plasma Heating and Electrons Acceleration
• On the estimate of magnetic non-potentiality of sunspots derived using Hinode SOT/SP observations: Effect of polarimetric noise
• Flux emergence and generation of flare-productive active regions
• Meridional flow in the solar polar caps revealed by magnetic field observation and simulation
• The dynamic chromosphere: pushing the boundaries of observations and models
• Formation of a solar Ha filament from orphan penumbrae
• Empirical determination of atomic line parameters of the 1.5 $\mu$m spectral region
• No universal connection between the vertical magnetic field and the umbra-penumbra boundary in sunspots
• Small-scale magnetic flux emergence preceding a chain of energetic solar atmospheric events
• Detection of Supergranulation Alignment in Polar Regions of the Sun by Helioseismology
• Supersonic Evershed flow outside Sunspots
• Driving solar coronal MHD simulations on high-performance computers
• Effects of unresolved magnetic field on Fe I 617.3 and 630.2 nm line shapes
• Evolution of exploding granules from coordinated observations by THEMIS, IRIS, SDO/HMI, and HINODE, and a simulation
• The role of the chromospheric magnetic canopy in the formation of a sunspot penumbra
• Observations of solar scattering polarization at high spatial resolution
• Photospheric downward plasma motions in the quiet-Sun
• Simultaneous ALMA-Hinode-IRIS observations on footpoint signatures of a soft X-ray loop-like microflare
• Instrument-To-Instrument translation: Instrumental advances drive restoration of solar observation series via deep learning
• Probing Upflowing Regions in the Quiet Sun and Coronal Holes
• Opacity distribution functions for stellar spectra synthesis
• Spectroscopy at the solar limb: II. Are spicules heated to coronal temperatures ?
• The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III
• Long-term variation of the solar polar magnetic fields at different latitudes
• Estimating the rate of field line braiding in the solar corona by photospheric flows
• A Non-Linear Magnetic Field Calibration Method for Filter-Based Magnetographs by Multilayer Perceptron
• Evidence for Partial Taylor Relaxation from Changes in Magnetic Geometry and Energy during a Solar Flare
• Large-Scale Spatial Cross-Calibration of Hinode/SOT-SP and SDO/HMI
• Photospheric downflows observed with SDO/HMI, HINODE, and an MHD simulation
• A novel inversion method to determine the coronal magnetic field including the impact of bound-free absorption
• On measuring divergence for magnetic field modeling
• A Deep Learning Approach to Generating Photospheric Vector Magnetograms of Solar Active Regions for SOHO/MDI Using SDO/HMI and BBSO Data
• Fast Magnetosonic Waves and Flows in a Solar Prominence Foot: Observations and Modeling
• Space-Time Distribution of G-Band and Ca II H-Line Intensity Oscillations in Hinode/SOT-FG Observations
• Contribution to the modeling of solar spicules
• Penumbral micro-jets at high spatial and temporal resolution
• Investigating the effect of solar ambient and data characteristics on Ca II K observations and line profile measurements
• Formation Heights of Extreme Ultraviolet Lines in an Active Region Derived by Correlation of Doppler Velocity and Magnetic Field
• MHD Simulation of Homologous Eruptions from Solar Active Region 10930 Caused by Sunspot Rotation
• Solar Polar Flux Redistribution based on Observed Coronal Holes
• Wave propagation in a solar quiet region and the influence of the magnetic canopy
• A spectral optical flow method for determining velocities from digital imagery
• Calibration of full-disk He I 10830 Å filtergrams of the Chromospheric Telescope
• Connecting the Wilson depression to the magnetic field of sunspots
• Probability Distribution Functions of Sunspot Magnetic Flux
• Flaring together: A preferred angular separation between sympathetic flares on the Sun
• On the Response of the Transition Region and the Corona to Rapid Excursions in the Chromosphere
• Strongest coronal magnetic fields in solar cycles 23-24: probing, statistics, and implications
• The effect of spatial sampling on magnetic field modeling and helicity computation
• Evolution of Stokes V area asymmetry related to a quiet Sun cancelation observed with GRIS/IFU
• Acoustic Events in the Solar Atmosphere from Hinode/SOT NFI observations
• Chromospheric impact of an exploding solar granule
• Interaction and Eruption of Two Filaments Observed by Hinode, SOHO, and STEREO
• Observational Evidence for Coronal Twisted Flux Rope
• Magnetic Structure of Umbral Dots Observed with Hinode Solar Optical Telescope
• Helioseismic Signature of Chromospheric Downflows in Acoustic Travel-Time Measurements from Hinode
• The Relationship between Solar Coronal X-Ray Brightness and Active Region Magnetic Fields: A Study Using High Resolution Hinode Observations
• Observation of kink waves and their reconnection-like origin in solar spicules
• Ca II K Spectral Study of an Emerging Flux Region using Domeless Solar Telescope in Hida Observatory
• Statistical Analysis of Current Helicity and Twist in Solar Active Regions over the Phases of the Solar Cycle Using the Spectro-Polarimeter Data of Hinode
• Spectro-polarimetric simulations of the solar limb: absorption-emission FeI $6301.5\mathring{\mathrm{A}}$ and $6302.5\mathring{\mathrm{A}}$ line profiles and torsional flows in the intergranular magnetic flux concentrations
• A new view on exoplanet transits: Transit of Venus described using three-dimensional solar atmosphere Stagger-grid simulations
• Two Types of Dynamic Cool Coronal Structures Observed with STEREO and HINODE
• Variations of magnetic bright point properties with longitude and latitude as observed by Hinode/SOT G-band data
• Thermodynamic evolution of a sigmoidal active region with associated flares
• Characteristics and Evolution of the Magnetic field and Chromospheric Emission in an Active Region Core Observed by Hinode
• Probing the quiet solar atmosphere from the photosphere to the corona
• Continuum enhancements, line profiles and magnetic field evolution during consecutive flares
• Solar-cycle and Latitude Variations in the Internetwork Magnetism
• The polarization signature of photospheric magnetic fields in 3D MHD simulations and observations at disk center
• Observed Effect of Magnetic Fields on the Propagation of Magnetoacoustic Waves in the Lower Solar Atmosphere
• Investigating the relation between sunspots and umbral dots
• Evolution Of Downflows In The Transition Region Above A Sunspot Over Short Time-Scales
• Vector Magnetic Fields and Current Helicities in Coronal Holes and Quiet Regions
• Retrieval of solar magnetic fields from high-spatial resolution filtergraph data: the Imaging Magnetograph eXperiment (IMaX)
• A nonlinear solar magnetic field calibration method for the filter-based magnetograph by the residual network
• About the directional properties of Solar Spicules from Hough Transform analysis
• A study of the capabilities for inferring atmospheric information from high-spatial-resolution simulations
• Expulsion of counter Evershed flows from sunspot penumbrae
• Study of the Dynamics of Convective Turbulence in the Solar Granulation by Spectral Line Broadening and Asymmetry
• Centre-to-limb properties of small, photospheric quiet Sun jets
• Sunspot Bright Points
• Photospheric Flow Field Related to the Evolution of the Sun's Polar Magnetic Patches Observed by Hinode SOT
• Dynamics in the transition region beneath active region upflows viewed by IRIS
• Scales of the magnetic fields in the quiet Sun
• Four decades of advances from MSDP to S4I and SLED imaging spectrometers
• Small-scale dynamic phenomena associated with interacting fan-spine topologies: quiet-Sun Ellerman bombs, UV brightenings, and chromospheric inverted-Y-shaped jets
• Temporal relations between magnetic bright points and the solar sunspot cycle
• Simulation of a Solar Jet Formed from an Untwisting Flux Rope Interacting with a Null Point
• A New Type of Jets in a Polar Limb of Solar Coronal Hole
• A Refined Model of Convectively-Driven Flicker in Kepler Light Curves
• Morphological study of penumbral formation
• Probable identification of the on-disk counterpart of spicules in Hinode Ca II H observations
• The MODEST catalog of depth-dependent spatially coupled inversions of sunspots observed by Hinode/SOT-SP
• Fractal multi-scale nature of solar/stellar magnetic field
• Evidence of quiet Sun chromospheric activity related to an emerging small-scale magnetic loop
• On the line profile changes observed during the X2.2 class flare in the active region NOAA 11158
• Infrared diagnostics of the solar magnetic field with Mg I 12 $\mu$m lines: forward-model results
• Acoustic Power Absorption and its Relation with Vector Magnetic Field of a Sunspot
• Analysis of horizontal flows in the solar granulation
• Nonlinear Fast Magnetosonic Waves in Solar Prominence Pillars
• Fundamental Transverse Vibrations of the Active Region Solar Corona
• Chromospheric plasma ejection above a pore
• Temporal evolution of short-lived penumbral microjets
• On the 5-Minute Oscillations of Photospheric and Chromospheric Swirls
• Towards Spectroscopically Detecting the Global Latitudinal Temperature Variation on the Solar Surface
• Comprehensive Determination of the Hinode/EIS Roll Angle
• A Search for High-Frequency Coronal Brightness Variations in the 21 August 2017 Total Solar Eclipse
• Internetwork Magnetic Fields Seen in Fe I 1564.8 nm
• A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842 I. Dynamics of the Solar Eruption Associated with the X7.1 Solar Flare
• Evidences to the pulse like origin of double spicules based on Hinode/SOT observations
• The dynamics of AR 12700 in its early emerging phase I: interchange reconnection
• Oscillations in solar Jets Observed with the SOT of Hinode: Viscous Effects during Reconnection
• Spicules in IRIS Mg II Observations: Automated Identification
• Magnetic Field Structures in a Facular Region Observed by THEMIS and Hinode
• Association of calcium network bright points with underneath photospheric magnetic patches
• The role of the Lorentz force in sunspot equilibrium
• Estimating electric current densities in solar active regions
• Inversion of Zeeman polarization for solar magnetic field diagnostics
• Global impact of emerging internetwork fields on the low solar atmosphere
• Improved SOT (Hinode mission) high resolution solar imaging observations
• Fast Mid-IR Flashes Detected During Small Solar X-Ray Bursts
• The Role of a Tiny Brightening in a Huge Geo-effective Solar Eruption Leading to the St Patrick's Day Storm
• Determining the Magnetic Field in the Atmosphere of a Solar Active Region Observed by the CLASP2.1 Sounding Rocket Experiment
• Penumbral brightening events observed in AR NOAA 12546
• Calcium bright knots and the formation of chromospheric anemone jets on the Sun
• On Making Magnetic-Flux-Rope $\Omega$ Loops for Solar Bipolar Magnetic Regions of All Sizes by Convection Cells
• Analysis of Pseudo-Lyapunov Exponents of Solar Convection Using State-of-the-Art Observations
• Sustained heating of the chromosphere and transition region over a sunspot light bridge
• Spectral resolution effects on the information content in solar spectra
• EIS/Hinode observations of Doppler flow seen through the 40 arcsec wide slit
• The dynamics of AR 12700 in its early emerging phase II: fan-shaped activities relevant to arch filament systems
• Spectropolarimetric diagnostics of unresolved magnetic fields in the quiet solar photosphere
• Statistical Study of Emerging Flux Regions and the Upper Atmosphere Response
• Confinedness of an X3.1 class solar flare occurred in NOAA 12192: Analysis from multi-instruments observations
• Statistical properties of spicules in MURaM-ChE
• Wavelength Dependence of Image Quality Metrics and Seeing Parameters and their Relation to Adaptive Optics Performance
• Proper Motions of Sunspots' Umbral Dots at High Temporal and Spatial Resolution
• Deriving Potential Coronal Magnetic Fields from Vector Magnetograms
• A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare
• Seismological determination of the Alfvén speed and plasma-beta in solar photospheric bright points
• Center to limb variation of penumbral Stokes V profiles
• New Types of the Chromospheric Anemone Microflares: Case Study
• Fine Magnetic Characteristics of a Light Bridge by Hinode
• Shock-Cloud Interaction in the Solar Corona
• Temporal Relation between Disappearance of Penumbral Fine-Scale Structure and Evershed Flow
• Super Penumbral Chromospheric Flare
• High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS)
• Superstrong magnetic fields in sunspot bipolar light bridges
• Topological model of the anemone microflares in the solar chromosphere
• Size matters
• Magnetic properties of orphan penumbrae
• ALMA Observations of Solar Spicules in a Polar Coronal Hole
• A new view of the solar interface region from the Interface Region Imaging Spectrograph (IRIS)
• Solar photospheric velocities measured in space: a comparison between SO/PHI-HRT and SDO/HMI
• Instrumental and Observational Artifacts in Quiet Sun Magnetic Flux Cance llation Functions
• Seeing-Induced Errors in Solar Doppler Velocity Measurements
• Observation of "Topological" Microflares in the Solar Atmosphere
• Evaluating Pointing Strategies for Future Solar Flare Missions
• Self-consistent numerical simulations for the formation and dynamics of solar prominences
• A High-resolution, Inversion-Based Synoptic Study of Solar Granulation
• First detection of sign-reversed linear polarization from the forbidden [O I] 630.03 nm line
• Categorization model of moving small-scale intensity enhancements in solar active regions
• Are the photospheric sunspots magnetically force-free in nature?
• Least-Squares Fitting Methods for Estimating the Winding Rate in Twisted Magnetic-Flux Tubes
• Velocity fields in and around sunspots at the highest resolution
• Emergence of magnetic flux sheets in the quiet Sun. I. Statistical properties
• Statistical Studies of Solar White-Light Flares and Comparisons with Superflares on Solar-type Stars
• Observations of Photospheric Magnetic Structure below a Dark Filament using the Hinode Spectro-Polarimeter
• Image instabilities and polarization cross-talk
• Atmosphere above a large solar pore
• A stray light analysis for SO/PHI-HRT and an updated comparison of the inferred magnetic field with SDO/HMI
• Mode coupling in solar spicule oscillations
• Chirality and magnetic configuration associated with two-ribbon solar flares: AR 10930 versus AR 11158
• Exploiting solar visible-range observations by inversion techniques: from flows in the solar subsurface to a flaring atmosphere
• Evolution of twist-shear and dip-shear in Faring active region NOAA 10930
• Distribution of Magnetic Shear Angle in an Emerging Flux Region
• The multi-thermal chromosphere: inversions of ALMA and IRIS data
• A publicly available multi-observatory data set of an enhanced network patch from the Photosphere to Corona
• Fields and Flares: Understanding the Complex Magnetic Topologies of Solar Active Regions
• Cloud model inversions of strong chromospheric absorption lines using principal component analysis
• Compression Method for Solar Polarization Spectra Collected from Hinode SOT/SP Observations
• The NWRA Classification Infrastructure: Description and Extension to the Discriminant Analysis Flare Forecasting System (DAFFS)
• Polarization calibration of the Tandem Etalon Magnetograph of the Solar Magnetic Activity Research Telescope at Hida Observatory
• An analytical model of prominence dynamics
• Relationship between magnetic field properties and statistical flow using numerical simulation and magnetic feature tracking on solar photosphere
• A comparison of measured and simulated solar network contrast
• Rotational radial shear in the low solar photosphere. Direct detection from high-resolution spectro-imaging
• Similarities of magnetoconvection in the umbra and in the penumbra of sunspots