Solar Physics

Papers
(The median citation count of Solar Physics is 2. 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 2021-11-01 to 2025-11-01.)
ArticleCitations
Rate of Change of Large-Scale Solar-Wind Structure86
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube61
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit48
Numerical Simulation of Longitudinal Oscillation of Filament Based on Smoothed Particle Hydrodynamics (SPH) Method38
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S34
Fabry–Pérot Interferometer-Based Tunable Narrow-Band Imager for Solar Chromospheric Observation: First Results34
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events32
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data28
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data28
The Mean Temperatures of CME-Related Dimming Masses24
Observations of Switchback Chains in a Twin-CME Event24
CME-Flare Association and the Role of Reconnection in CME Acceleration24
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 177724
Avalanching Together: A Model for Sympathetic Flaring24
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”23
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions23
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images23
Correction to: Kanzelhöhe Observatory: Instruments, Data Processing and Data Products21
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2421
Accelerating Multiframe Blind Deconvolution via Deep Learning21
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200320
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind20
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes19
Solar Filament Segmentation Based on Improved U-Nets19
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 2418
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery18
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning18
Potential Field Source Surface and Non-linear Force-Free Field Extrapolation to Model Magnetic Field Structure for a Giant Solar Filament16
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution16
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology16
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations15
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy15
Linear Correlation Between Radial and Normal Component Fluctuations of the Interplanetary Magnetic Field15
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions15
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series15
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)15
Forecasting Solar Flares by Data Assimilation in Sandpile Models14
MHD Simulations of CME with Associated Prominence Eruption14
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD14
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles13
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components13
Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope13
An Efficient Method for Magnetic Field Extrapolation Based on a Family of Analytical Three-Dimensional Magnetohydrostatic Equilibria12
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts12
The Future of Solar Modelling: Requirements for a New Generation of Solar Models12
Lifetime of Sunspots and Pores11
Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind11
Deciphering Solar Magnetic Activity: 140 Years of the ‘Extended Solar Cycle’ – Mapping the Hale Cycle11
Predicting Solar Cycle 26 Using the Polar Flux as a Precursor, Spectral Analysis, and Machine Learning: Crossing a Gleissberg Minimum?11
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions11
An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data11
Corotating Interaction Regions during Solar Cycle 24: A Study on Characteristics and Geoeffectiveness11
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial11
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma11
Detections of Multi-Periodic Oscillations During a Circular Ribbon Flare11
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data11
Solar Flare Effects on the Earth’s Lower Ionosphere11
Structures of Various Types of Symmetry in the Solar Activity Cycle10
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope10
IRIS Observational Approach to the Oscillatory and Damping Nature of Network and Internetwork Chromosphere Small-Scale Brightening (SSBs) and Their Unusual Dynamical and Morphological Differences in D10
Fabry-Pérot Interferometer Based Imaging Spectrometer for Fe I Line Observation and Line-of-Sight Velocity Measurement10
Propagating Oscillations in the Lower Atmosphere Under Coronal Holes10
Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms Using the uGMRT9
Application of a Neural Network for Identifying Erroneous Solar Images9
Sunspots Identification Through Mathematical Morphology9
The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles9
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)9
A Multi-Viewpoint CME Catalog Based on SoloHI Observed Events9
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability9
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission9
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions9
A Synchronized Two-Dimensional $\alpha $–$\Omega $ Model of the Solar Dynamo9
Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model9
Multiscale Aspects of the Solar Indexes Mg II, F10.7 and Sunspot Number9
Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts9
Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona9
Improvements to the Empirical Solar Wind Forecast (ESWF) model8
Correction to: On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis8
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique8
Heliolatitudinal Distribution and Hemispheric Asymmetry of Source Locations for Super Geomagnetic Storms (Dst ≤−250 nT) During Different Phases of Solar Cycles8
Observation of a Flare and Filament Eruption in Lyman-$\alpha $ on 8 September 2011 by the PRoject for OnBoard Autonomy/Large Yield Radiometer (PROBA2/LYRA)8
Time Lag Between Cosmic-Ray and Solar Variability: Sunspot Numbers and Open Solar Magnetic Flux8
The “SEP Clock”: A Discussion of First Proton Arrival Times in Wide-Spread Solar Energetic Particle Events8
Tidally Synchronized Solar Dynamo: A Rebuttal8
Flare Energetics, CME Launch and Heliospheric Propagation for the May 2024 Events, as Derived from Ensemble MHD Modelling8
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)8
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.78
Correction to: Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 248
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19698
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations8
Modelling Persistent Cycles in Solar Activity8
Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms ($\mathrm{Dst} \le -100$ nT) from 1932 to 20188
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 248
Adding Further Pieces to the Synchronization Puzzle: QBO, Bimodality, and Phase Jumps8
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images7
Short and Intermediate Periodicities in Ca ii K Plage Areas as Seen in Kodaikanal Images for Individual Cycles from 14 to 227
Clarifying Physical Properties of Magnetic Fields in Sunspots7
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter7
Aditya-L1 - An Observatory Class Mission: Spacecraft, Mission, and Operations7
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon7
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos7
Correction to: Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances7
HelioIndex: A Directory of Active Researchers in Solar and Heliospheric Physics7
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles7
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence7
Sunspot Rotation in High- and Low-Flaring Active Regions7
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20217
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe7
Kinematic Study of Radio-Loud CMEs Associated with Solar Flares and DH Type-II Radio Emissions During Solar Cycles 23 and 247
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis7
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation7
Data-Driven Forecasting of Sunspot Cycles: Pros and Cons of a Hybrid Approach7
Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns?7
Meridional Movements of Individual Sunspots and Pores7
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes7
Differential Rotation of Solar Filaments Early Observed by the OGAUC in the Period 1929 – 19417
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere6
Turbulence in Sources of Decimetric Flare Continua6
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle6
A Stellar View of the Sun6
On the Estimation of the SHARP Parameter MEANALP from AIA Images Using Deep Neural Networks6
Properties of EUV Imaging Spectrometer (EIS) Slot Observations6
The Gondola for the Sunrise iii Balloon-Borne Solar Observatory6
Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption That Resulted in a Sustained Gamma Ray Emission Event6
Behaviour of 27-Day and 13.5-Day Periodicities in Galactic Cosmic Particles as Observed by Spacecraft and Neutron Monitors During Different Solar Polarity Cycles6
An Enhanced ResNet Model for Solar Activity Classification with Dual-Passband CHASE Data6
Long-Term Variation of Helioseismic Far-Side Images and What Causes It6
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”6
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques6
The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 20246
Polarimetric Studies of a Fast Coronal Mass Ejection6
Solar-Cycle Variability Results from the Solar Radiation and Climate Experiment (SORCE) Mission6
Probing Upflowing Regions in the Quiet Sun and Coronal Holes6
A Study on the Transition-Range Spectral Index of the Solar Wind Turbulence in the Inner Heliosphere6
Coronal Density Measurements Using Giant Radio Pulses of the Crab Pulsar at the Cycle 24/25 Minimum6
Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field6
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 246
Changing Methodologies in Solar Physics6
Solar Soft X-Ray Irradiance Variability, II: Temperature Variations of Coronal X-Ray Features6
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations6
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
Dynamics of Explosive Events Observed by the Interface Region Imaging Spectrograph6
Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 266
Quantifying Chromosphere Response to Flare Energy Release Using AIA Observations in 1600 Å and 304 Å Passbands6
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)6
Multi-Wavelength Observations of Quasi-Periodic Pulsations in a Solar Flare6
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20236
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)6
High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis5
A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI5
Solar Rotation in the Period 1611 – 1631 Determined Using Observations of Christoph Scheiner5
Correction to: A Discussion of Implausible Total Solar-Irradiance Variations Since 17005
Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission5
Disambiguation of Vector Magnetograms by Stereoscopic Observations from the Solar Orbiter (SO)/Polarimetric and Helioseismic Imager (PHI) and the Solar Dynamic Observatory (SDO)/Helioseismic and Magne5
Amplitudes of Solar Gravity Modes: A Review5
Alfvén Pulse in a Chromospheric Magnetic Tube and Generation of the Super-Dreicer Electric Field5
Accuracy Analysis of the On-board Data Reduction Pipeline for the Polarimetric and Helioseismic Imager on the Solar Orbiter Mission5
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code5
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 255
The Properties of Non-Potential Magnetic Field Parameters in a Super-Active Region with Complex Structures and Strong Solar Flares5
Improved Tomographic Reconstruction of 3D Global Coronal Density from STEREO/COR1 Observations5
Noise in Maps of the Sun at Radio Wavelengths II: Solar Use Cases5
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations5
The Narrow Field Imager (NFI) for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)5
Intense Geomagnetically Induced Currents (GICs): Association with Solar and Geomagnetic Activities5
Precursory Signs of Large Forbush Decreases: The Criterion of Anisotropy5
Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances5
A Comparison of Sparse and Non-sparse Techniques for Electric-Field Inversion from Normal-Component Magnetograms5
Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods5
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase5
Reply to “Response to ‘Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators’ by R.J. Booth”5
An MHD Study of Large-Amplitude Oscillations in Solar Filaments5
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132835
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter5
Synthetic Resonance and Thomson Scattering of a Chromospheric $\text{Ly}\alpha $ Profile Using the Bastille Day CME Model Corona: Part 15
The Role of Photospheric Magnetic Flux Diffusion in Initiation of Solar Eruptions5
Data Processing Pipeline of the SUTRI EUV Imager on the SATech-01 Satellite5
Annual Variations in the Near-Earth Solar Wind5
A New Global Nonlinear Force-Free Coronal Magnetic-Field Extrapolation Code Implemented on a Yin–Yang Grid5
Ripples and Rush-to-the-Poles in the Photospheric Magnetic Field5
Magnetic Field and Plasma Diagnostics for Solar Coronal Mass Ejections: A Case Study Using the Forward Modeling Approach5
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Models of Collisionless Quasineutral Solar Wind Current Sheets5
Solar Irradiance Spectra from the Compact SOLSTICE (CSOL) Experiment: Instrument Design, FUV Calibration, Measurements, and Comparison of the 2018 Rocket Flight5
A Study on Correcting the Effect of Polarization Crosstalk in Full-Disk Solar Photospheric Magnetic Field Observations5
Similarities and Differences of SARs in Solar Cycle 244
Long-Term Trend Analysis in the Solar Radiation and Climate Experiment (SORCE)/Spectral Irradiance Monitor (SIM)4
On the Most Interesting Solar-Wind and Cosmic-Ray Events in February–April 20234
The Sun’s Large-Scale Flows I: Measurements of Differential Rotation & Torsional Oscillation4
CATEcor: An Open Science, Shaded-Truss, Externally-Occulted Coronagraph4
How Hot Can Small Solar Flares Get?4
Detection of “Diffuse” Coronal He I 1083 During the April 8, 2024 Solar Eclipse: Evidence for Terrestrial Atmospheric Scattering Contribution4
Solar-Filament Detection and Classification Based on Deep Learning4
The Sun’s Non-Potential Corona over Solar Cycle 244
Hydrogen Ionization Inside the Sun4
The Hazard of UV-Induced Oxidation to Solar-Viewing Spacecraft Optics4
Quasi-Separatrix Layers and Three-Dimensional Magnetic Reconnection: Theory and Observations of Solar Flares (Invited Review)4
Spectral Analysis of Rieger Periodicity Behaviour in O and Fe Galactic Cosmic Particles Observed by ACE in Solar Cycles 23 and 244
Coronal Electric Currents and Kink Instability of Magnetic Flux Rope4
Solar Active Regions Detection and Tracking Based on Deep Learning4
Properties of Type-II Radio Bursts in Relation to Magnetic Complexity of the Solar Active Regions4
Periodic Variation of Anomalous Cosmic Ray Oxygen During Solar Cycles 23 and 244
Solar Low Energy X-ray Spectrometer (SoLEXS) on Board Aditya-L1 Mission4
Analysis of Galactic Cosmic Ray Anisotropy During the Time Period from 1996 to 20204
Nonlinear Propagating Slow Waves in Cooling Coronal Magnetic Loops4
Visible Emission Line Coronagraph (VELC) on Board Aditya-L14
Comparison of Polar Magnetic Fields Derived from MILOS and MERLIN Inversions with Hinode/SOT-SP Data4
Distributions of Mesoscale Periodic Structures in the Elemental and Ionic Composition of the Solar Wind4
Data-Constrained Magnetohydrodynamics Simulation of a Confined X-Class Flare in NOAA Active Region 111664
First Hard X-Ray Imaging Results by Solar Orbiter STIX4
Anticipating Solar Flares4
Reconstruction of Carrington Rotation Means of Open Solar Flux over the Past 154 Years4
Correction to: Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods4
The First Survey of Quiet Sun Features Observed in Hard X-Rays with NuSTAR4
Systems Approach to Polarization Calibration for the Daniel K. Inouye Solar Telescope (DKIST)4
Observations of Flare Induced Doppler Shifts in the Si iii 1206 Å Line4
Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager4
Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection4
Localization of the Gamma-Ray Emission Region in the 1 September 2014 Behind-the-Limb Solar Flare According to the Fermi/LAT Data3
A New Solar Hard X-ray Image Reconstruction Algorithm for ASO-S/HXI Based on Deep Learning3
Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism3
Correction to: Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions3
Direct Observational Evidence of Solar Wind Density Controlling the Evolution of the Ring Current During the 2024 October Major Storm3
Temporal and Latitudinal Variation in Penumbra-Umbra Ratios of the Sunspots: Analyses of RGO, Kodaikanal and Debrecen Databases3
The Tautenburg Solar Laboratory (TauSoL) as Pathfinder for SPRING3
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME3
Sympathetic Quiet and Active Region Filament Eruptions3
Tomography of the Solar Corona with the Metis Coronagraph II: Three-Dimensional Reconstructions of the Electron Density and Comparison with Reconstructions Based on LASCO-C23
Solar Radio Burst Prediction Based on a Multimodal Model3
Forecasting Shock-Associated Energetic Particle Intensities in the Inner Heliosphere: A Proof-of-Concept Capability for the PUNCH Mission3
On the Hierarchical Relationship Between Type-II Radio Bursts and the Associated Coronal Mass Ejections3
New Anisotropic Cosmic-Ray Enhancement (ACRE) Event on 5 November 2023 Due to Complex Heliospheric Conditions3
SOLar-STellar Irradiance Comparison Experiment II (SOLSTICE II): End-of-Mission Validation of the SOLSTICE Technique3
Statistical Analysis of Sunspot Area and Magnetic Flux on Solar Disc During 2011 – 20233
Comparison of Relative Magnetic Helicity Flux Calculation Results Based on the Line-of-Sight Magnetograms of ASO-S/FMG and SDO/HMI3
On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis3
The Solar Radiation and Climate Experiment (SORCE) Mission: Final Calibrations and Data Products3
A Statistical Study of Solar White-Light Flares Observed by the White-Light Solar Telescope of the Lyman-Alpha Solar Telescope on the Advanced Space-Based Solar Observatory (ASO-S/LST/WST) at 360 nm3
Subsurface Horizontal Flows During Solar Cycles 24 and 25 with Large-Tile Ring-Diagram Analysis3
Wide-Field Image Restoration of G-Band and Ca ii K Images Containing Large and Complex Active Regions3
Forecasting the Dst Index with Temporal Convolutional Network and Integrated Gradients3
Origin of the Solar Rotation Harmonics Seen in the EUV and UV Irradiance3
Magnetic Field and Density Models in the Zebra Source Region3
Multiwavelength Observations of Quasiperiodic Pulsations in the Impulsive Phase of an Eruptive Flare with the Hard X-Ray Imager On Board ASO-S and Other Instruments3
Forecasting Solar Cycle 25 with Physical Model-Validated Recurrent Neural Networks3
Solar Flare Catalogue from 3 Years of Chandrayaan-2 XSM Observations3
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