Solar Physics

Papers
(The median citation count of Solar Physics is 1. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2021-02-01 to 2025-02-01.)
ArticleCitations
Numerical Simulation of Longitudinal Oscillation of Filament Based on Smoothed Particle Hydrodynamics (SPH) Method98
Energy Definition and Minimization in Avalanche Models for Solar Flares81
A Simple Radial Gradient Filter for Batch-Processing of Coronagraph Images60
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques39
The Temperature Dependence of Hot Prograde Flows in Solar Active Regions39
Energy Spectra vs. Element Abundances in Solar Energetic Particles and the Roles of Magnetic Reconnection and Shock Acceleration33
September 2017 Space-Weather Events: A Study on Magnetic Reconnection and Geoeffectiveness26
Super-Resolution of SOHO/MDI Magnetograms of Solar Active Regions Using SDO/HMI Data and an Attention-Aided Convolutional Neural Network26
A Diligent Analysis of the Flash and Coronal Spectrum of the Total Solar Eclipse of 20 March 201526
So Far, so Good — My First 82 Years25
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 2425
A Possible Connection between the de Vries Cycle and the Solar Dynamo25
A Theoretical Estimate of the Pole-Equator Temperature Difference and a Possible Origin of the Near-Surface Shear Layer25
Similarities and Differences of SARs in Solar Cycle 2425
How Magnetic Erosion Affects the Drag-Based Kinematics of Fast Coronal Mass Ejections24
The Advanced Space-Based Solar Observatory (ASO-S)23
Updates to the SUMER Spectral Atlas22
An Improved Method for Estimating the Velocity Field of Coronal Propagating Disturbances22
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle21
Separating the aa-index into Solar and Hale Cycle Related Components Using Principal Component Analysis20
Radial Distributions of Coronal Electron Temperatures: Specificities of the DYN Model19
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”19
Two New Methods for Counting and Tracking the Evolution of Polar Faculae18
Improvements of the Longitudinal Magnetic Field Measurement from the Solar Magnetic Field Telescope at the Huairou Solar Observing Station18
Editorial Appreciation18
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations17
Comparison of Line-of-Sight Magnetic Field Observed by ASO-S/FMG, SDO/HMI and HSOS/SMAT17
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 202317
Flux Calibration of Coronal Magnetic Field16
Effects of Initial Conditions on Magnetic Reconnection in a Solar Transient16
Behaviour of 27-Day and 13.5-Day Periodicities in Galactic Cosmic Particles as Observed by Spacecraft and Neutron Monitors During Different Solar Polarity Cycles16
Long-Term Variation of Helioseismic Far-Side Images and What Causes It16
Machine-Learning-Based Numerical Solution for Low and Lou’s Nonlinear Force-Free Field Equilibria16
Thermal Trigger for Solar Flares III: Effect of the Oblique Layer Fragmentation15
Study of Fine Radio-Burst Structures (FRBS) Observed by the Mexican Array Radio Telescope (MEXART)15
Rudolf Wolf to Alfred Wolfer: The Transfer of the Reference Observer in the International Sunspot Number Series (1876–1893)15
Characterization and Correction of the Scattering Background Produced by Dust on the Objective Lens of the Lijiang 10-cm Coronagraph15
The Mean Temperatures of CME-Related Dimming Masses14
Comparing the Heliospheric Cataloging, Analysis, and Techniques Service (HELCATS) Manual and Automatic Catalogues of Coronal Mass Ejections Using Solar Terrestrial Relations Observatory/Heliospheric I14
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit13
Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns?13
East–West Asymmetry in Interplanetary-Scintillation-Level Variation Associated with Solar-Wind Disturbances13
Comparison of Solar Activity Parameters and Associated Forbush Decreases in Solar Cycles 23 and 2413
Helio-latitude Dependence of the Solar Wind Parameters and the Magneto-Gravitational Dragging of the Solar Wind13
The Fibre Resolved OpticAl and Near-Ultraviolet Czerny–Turner Imaging Spectropolarimeter (francis)12
Transiting Exoplanet Survey Satellite (TESS) Observations of Flares and Quasi-Periodic Pulsations from Low-Mass Stars and Potential Impact on Exoplanets12
Comprehensive Characterization of the Dynamics of Two Coronal Mass Ejections in the Outer Corona12
Detection of Coronal Mass Ejections Using Unsupervised Deep Clustering12
Sunspot Rotation in High- and Low-Flaring Active Regions12
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption12
Solar Soft X-ray Irradiance Variability III: Magnetic Field Variations of Coronal X-ray Features12
CME-Flare Association and the Role of Reconnection in CME Acceleration12
Application of the Markov Chain Model to Sunspots and Solar Plages for the Period 1910 to 1937 Using Data from Ebro Catalogues12
Methodology for Predicting the Probability Distribution of the Amplitude of Solar Cycle 2512
Solar Soft X-Ray Irradiance Variability, II: Temperature Variations of Coronal X-Ray Features12
A Semi-Automatic Method to Measure the Rotation of Sunspots11
On the Periodicities in Solar Rotation and Activity Determined from Sunspot-Group Data and Possible Connection with Rossby-Like Waves11
Rate of Change of Large-Scale Solar-Wind Structure11
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events11
Kilometric Type II Radio Emissions in Wind/WAVES TNR Data and Association with Interplanetary Structures Near Earth10
Computation of Winding-Based Magnetic Helicity and Magnetic Winding Density for SHARP Magnetograms in Spherical Coordinates10
Polarization of the Corona Observed During the 2017 and 2019 Total Solar Eclipses10
Multiwavelength Observations of a Partial Filament Eruption on 13 June 201110
Forecasting Medium-Term F10.7 Using the Deep-Learning Informer Model10
Response to Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal”10
Parameter Effects on the Total Intensity of H i Ly$\alpha $ Line for a Modeled Coronal Mass Ejection and Its Driven Shock10
A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument10
Sunspot-Cycle Evolution of Major Periodicities of Solar Activity10
Exploring the Origin of Stealth Coronal Mass Ejections with Magnetofrictional Simulations9
Scale Transfer in 1849: Heinrich Schwabe to Rudolf Wolf9
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”9
GLE # 67 Event on 2 November 2003: An Analysis of the Spectral and Anisotropy Characteristics Using Verified Yield Function and Detrended Neutron Monitor Data9
A Modern Reconstruction of Richard Carrington’s Observations (1853–1861)9
Coronal Signatures of Flare Generated Fast-Mode Wave at EUV and Radio Wavelengths9
The Daniel K. Inouye Solar Telescope (DKIST)/Visible Broadband Imager (VBI)9
Fabry–Pérot Interferometer-Based Tunable Narrow-Band Imager for Solar Chromospheric Observation: First Results9
Accelerating Multiframe Blind Deconvolution via Deep Learning9
Segmentation of Coronal Features to Understand the Solar EUV and UV Irradiance Variability III. Inclusion and Analysis of Bright Points9
Flattening Index of the Solar Corona and the Sun’s Magnetic Field9
Properties and Energetics of Magnetic Reconnection: I. Evolution of Flare Ribbons9
Is the Subsurface Meridional Flow Zero at the Equator?9
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 20039
Assessing the Predictability of Solar Energetic Particles with the Use of Machine Learning Techniques8
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind8
Equation of State of the Kappa-Distributed Solar Wind Particles in the Earth’s Magnetopause8
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes8
How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes8
Magnetic Imbalance at Supergranular Scale: A Driving Mechanism for Coronal Hole Formation8
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere8
Problems in Observation and Identification of Torsional Waves in the Lower Solar Atmosphere8
Solar Filament Segmentation Based on Improved U-Nets8
Comparing the Correlations Between Solar Cycle Parameters in the Northern and Southern Hemispheres8
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube8
Generating Photospheric Vector Magnetograms of Solar Active Regions for SOHO/MDI Using SDO/HMI and BBSO Data with Deep Learning8
Mancha3D Code: Multipurpose Advanced Nonideal MHD Code for High-Resolution Simulations in Astrophysics8
Daytime Sky Brightness at Dome C, Antarctica: Results from All ESCAPE Campaigns7
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S7
Origin of the Chromospheric Umbral Waves in Sunspots7
Enhancing Solar Cycle 25 and 26 Forecasting with Vipin-Deep-Decomposed-Recomposed Rolling-window (vD2R2w) Model on Sunspot Number Observations7
Characterizing High-Energy Solar Proton Events with Energies Below and Above 100 MeV7
Correction to: Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions7
Correction to: Kanzelhöhe Observatory: Instruments, Data Processing and Data Products7
Acoustic Waves in a High-Temperature Plasma III. Two-Periodic Disturbances7
Resonant Damping of Kink Modes in Solar Coronal Slabs7
A Diffraction Effect Investigation for the Solar Irradiance Absolute Radiometer on the Fengyun-3F Satellite7
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions7
Energy Partition in Four Confined Circular-Ribbon Flares6
Analysis of Overtones in Transverse Oscillations of Coronal Loops of an Active Region6
On the Instrumental Discrepancies in Lyman-Alpha Observations of Solar Flares6
Correction to: Global-Mode Analysis of Full-Disk Data from the Michelson Doppler Imager and the Helioseismic and Magnetic Imager6
Subsurface Horizontal Flows During Solar Cycles 24 and 25 with Large-Tile Ring-Diagram Analysis6
Automatic Detection of Occulted Hard X-Ray Flares Using Deep-Learning Methods6
Searching for a Solar Source of Magnetic-Field Switchbacks in Parker Solar Probe’s First Encounter6
North–South Asymmetry of Solar Meridional Circulation and Synchronization: Two Rings of Four Coupled Oscillators6
Cornelis de Jager: In Memoriam6
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles6
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images6
Helioseismic Constraints: Past, Current, and Future Observations6
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 246
Feasibility Study of Measuring Degree of Linear Polarization of the Solar F-Corona Using Filter Observations on the COronal Diagnostic EXperiment6
Observation of an Extraordinary Type V Solar Radio Burst: Nonlinear Evolution of the Electron Two-Stream Instability6
Reduced Microwave Brightness Temperature in a Sunspot Atmosphere Due to Open Magnetic Fields6
Derived Electron Densities from Linear Polarization Observations of the Visible-Light Corona During the 14 December 2020 Total Solar Eclipse6
The Effect of Missing Groups in the Calculation of the Solar Irradiance Deficit6
The Visible Spectro-Polarimeter of the Daniel K. Inouye Solar Telescope6
Catastrophic Cooling Instability in Optically Thin Plasmas6
A Discussion of Implausible Total Solar-Irradiance Variations Since 17006
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)6
The Evolution of Multipole Moments for the Global Solar Magnetic Field6
Impact of Magnetic and Flow Fields on Penumbrae and Light Bridges of Three Leading Sunspots in an Active Region6
The KIS Science Data Centre6
Coronal Density Measurements Using Giant Radio Pulses of the Crab Pulsar at the Cycle 24/25 Minimum6
Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity5
Four Decades of Advances from MSDP to S4I and SLED Imaging Spectrometers5
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution5
On the Nature of the Kink MHD Waves in Flowing and Twisted Coronal Flux Tubes5
Rediscovery of 23 Historical Records of Naked-Eye Sunspot Observations in AD 16185
A New Solar Hard X-ray Image Reconstruction Algorithm for ASO-S/HXI Based on Deep Learning5
Solar Rotation Multiples in Space-Weather Effects5
Multi-Spacecraft Observations of an Interplanetary Coronal Mass Ejection Interacting with Two Solar-Wind Regimes Observed by the Ulysses and Twin-STEREO Spacecraft5
Nature and Variability of the Electron Velocity Distribution Functions and the Nonequilibrium Boltzmann Entropy in the Solar Wind at the First Lagrangian (L1) Point During the Halo CME Event on 25 Jul5
Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?5
Temporal and Latitudinal Variation in Penumbra-Umbra Ratios of the Sunspots: Analyses of RGO, Kodaikanal and Debrecen Databases5
The New HELLRIDE at the Vacuum Tower Telescope5
Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field5
Multi-Wavelength Observations of Quasi-Periodic Pulsations in a Solar Flare5
Editorial Appreciation5
Solar Wind Discontinuity Interaction with the Bow Shock: Current Density Growth and Dawn-Dusk Asymmetry5
Origin of the Solar Rotation Harmonics Seen in the EUV and UV Irradiance5
Testing the Accuracy of Coimbra Astronomical Observatory Solar Filament Historical Series (1929–1941)5
Characteristics of Suprathermal Electrons in Small-Scale Magnetic Flux Ropes and Their Implications on the Magnetic Connection to the Sun5
Improved Approach in the Coupling Function Between Primary and Ground Level Cosmic Ray Particles Based on Neutron Monitor Data5
Analysis of the Solar Flare Index for Solar Cycles 18 – 24: Extremely Deep Gnevyshev Gap in the Chromosphere5
A Study on the Various Modes of Parallel Heat Conduction in the Coronal Loops of Small and Large Solar Flares Using Scaling Laws5
Oscillation Dynamics in Short-Lived Facular Regions During Their Lifetime5
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)5
Probing Upflowing Regions in the Quiet Sun and Coronal Holes5
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology5
Precursory Signals of Forbush Decreases Not Connected with Shock Waves5
Seeing Measurements with the Merak H$\upalpha$ Telescope5
Automated Detection of Accelerating Solar Eruptions Using Parabolic Hough Transform5
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning5
Turbulence in Sources of Decimetric Flare Continua5
Forecasting Shock-Associated Energetic Particle Intensities in the Inner Heliosphere: A Proof-of-Concept Capability for the PUNCH Mission5
The Instantaneous Response of the Geomagnetic Field, Near-Earth IMF, and Cosmic-Ray Intensity to Solar Flares5
Study of Temporal Profile and Flux Variation of GLE Events During Solar Cycles 23 and 24 Using GOES Data5
Response to “Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators” by R. Booth5
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. I. Kinematic Challenges5
Forecasting Solar Flares by Data Assimilation in Sandpile Models4
Exploring Standing and Reflected Slow-Mode Waves in Flaring Coronal Loops: A Parametric Study Using 2.5D MHD Modeling4
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components4
Migrating Dynamo Waves and Consequences for Stellar Current Sheets4
An Interesting Correlation Between the Peak Slope and Peak Value of a Sunspot Cycle4
Monochromatic Two-Fluid Alfvén Waves in the Partially Ionised Solar Chromosphere4
Modeling Global Magnetic-Flux Emergence in Bipolar Solar-Active Regions4
Statistical Analysis of Interplanetary Shocks from Mercury to Jupiter4
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions4
Longitudinal Plasma Motions Generated by Shear Alfvén Waves in Plasma with Thermal Misbalance4
Solar Radio-Burst Forecast Based on a Convolutional Neural Network4
A Linear Analysis of Torsional Alfvén Waves in Open Twisted Divergent Magnetic Flux Tubes for Coronal Heating4
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 244
Hemispheric Sunspot Numbers from the Astronomical Observatory of the University of Valencia (1940 – 1956)4
The Dispersion Relation for Waves in a Magnetic Flux Tube4
The Spectro-Polarimeter of the Andrei B. Severny Solar Tower Telescope at the Crimean Astrophysical Observatory: Optical Design and Implementation4
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD4
Using Flare-Induced Modulation of Three- and Five-Minute Oscillations for Studying Wave Propagation in the Solar Atmosphere4
Aurora Observations from the Principality of Transylvania from the 16th to the 18th Century CE4
Automated Sunspot Detection as an Alternative to Visual Observations4
Observation of Alfvén Waves in an ICME-HSS Interaction Region4
Spatial and Temporal Distribution of Solar Green-Line Corona for Solar Cycles 18 – 244
Solar Electron Beam Velocities That Grow Langmuir Waves in the Inner Heliosphere4
Sunspot Observations at the Eimmart Observatory: Revision and Supplement4
Slow Magnetoacoustic Waves in Smoothly Nonuniform Coronal Plasma Structures4
Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism4
Motion Magnification in Solar Imaging Data Sequences in the Sub-pixel Regime4
The Polar Field Reversal Process over Five Solar Cycles4
Near-Earth High-Speed and Slow Solar Winds: A Statistical Study on Their Characteristics and Geomagnetic Impacts4
Stokes Inversion Techniques with Neural Networks: Analysis of Uncertainty in Parameter Estimation4
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery4
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations4
Solar Event Detection Using Deep-Learning-Based Object Detection Methods4
A Reanalysis of the Number of Sunspot Groups Recorded by Pierre Gassendi in the Cycle Before the Maunder Minimum4
An Improved Prediction of Solar Cycle 25 Using Deep Learning Based Neural Network4
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions3
Center–Limb Variation of Solar Photospheric Microturbulence3
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)3
Sympathetic Quiet and Active Region Filament Eruptions3
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations3
Extreme Space-Weather Events and the Solar Cycle3
Plasma Heating in an Erupting Prominence Detected from Microwave Observations with the Siberian Radioheliograph3
The Greatest GOES Soft X-ray Flares: Saturation and Recalibration over Two Hale Cycles3
Forecasting Solar Cycle 25 with Physical Model-Validated Recurrent Neural Networks3
SOLar-STellar Irradiance Comparison Experiment II (SOLSTICE II): End-of-Mission Validation of the SOLSTICE Technique3
Accurate Short-Characteristics Radiative Transfer in A Numerical Tool for Astrophysical RESearch (ANTARES)3
Spectroscopy of Electric-Field Oscillations in the Solar Wind During the Passage of a Type III Radio Burst Using Observations Compared with Self-Similar Theory3
Hemispheric Sunspot Number Prediction for Solar Cycles 25 and 26 Using Spectral Analysis and Machine Learning Techniques3
Correction for the Weakening Magnetic Field Within the Sunspot Umbra Observed by ASO-S/FMG3
On the Estimation of the SHARP Parameter MEANALP from AIA Images Using Deep Neural Networks3
Solar Radio Burst Prediction Based on a Multimodal Model3
Cyclical Behavior of Magnetically Complex Sunspot Groups and Major Flares in Solar Cycles 22 – 243
Restoration of the K and F Components of the Solar Corona from LASCO-C2 Images over 24 Years [1996 – 2019]3
The Magnetic Power Spectra of Decaying Active Regions: New Evidence for the Large-Scale Magnetic Flux Bundle Submergence?3
Image Quality Specification for Solar Telescopes3
Correction to: The Fengyun-3E/Joint Total Solar Irradiance Absolute Radiometer: Instrument Design, Characterization, and Calibration3
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations3
Eruptive Flare, CME, and Shock Wave in the 25 August 2001 High-Energy Solar Event3
Interferometric Imaging, and Beam-Formed Study of a Moving Type-IV Radio Burst with LOFAR3
Solar Cycle Pairing and Prediction of Cycle 253
Conversion and Smoothing of MHD Shocks in Atmospheres with Open and Closed Magnetic Field and Neutral Points3
Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption3
A Stellar View of the Sun3
Solar Flare Prediction and Feature Selection Using a Light-Gradient-Boosting Machine Algorithm3
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data3
Thermal Trigger for Solar Flares II: Effect of the Guide Magnetic Field3
Gnevyshev Gap in the Large-Scale Magnetic Field3
Temporal Defocusing as a Depth Diagnostic of Submerged Sources of Transient Acoustic Emission from Solar Flares3
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME3
Effect of Thermal Conductivity, Compressive Viscosity and Radiative Cooling on the Phase Shift of Propagating Slow Waves with and Without Heating–Cooling Imbalance3
Correction to: Solar Temperature Variations Computed from SORCE SIM Irradiances Observed During 2003 – 20203
Observations of the Polarized Solar Corona During the Annular Eclipse of 14 October 20233
Solar-Cycle Variability Results from the Solar Radiation and Climate Experiment (SORCE) Mission3
Comparison Between Radio Loud and Radio Quiet Fast CMEs: A Reason for Radio Quietness3
Upflows in the Upper Solar Atmosphere3
Iterative Construction of the Optimal Sunspot-Number Series3
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series3
Rieger Periodicity Behaviour in Solar Mg ii 280 nm Spectral Emission3
Mitigation of Radio Frequency Interference in the Solar Radio Spectrum Based on Deep Learning3
Two Classes of Eruptive Events During Solar Minimum3
Error Estimation of Linear Polarization Data from Coronagraphs – Application to STEREO-A/SECCHI-COR1 Observations3
A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)2
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