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 2021-09-01 to 2025-09-01.)
ArticleCitations
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200380
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events57
Fabry–Pérot Interferometer-Based Tunable Narrow-Band Imager for Solar Chromospheric Observation: First Results45
Numerical Simulation of Longitudinal Oscillation of Filament Based on Smoothed Particle Hydrodynamics (SPH) Method40
Rate of Change of Large-Scale Solar-Wind Structure36
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube34
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit32
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2429
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions27
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”27
Accelerating Multiframe Blind Deconvolution via Deep Learning27
Correction to: Kanzelhöhe Observatory: Instruments, Data Processing and Data Products26
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 177724
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind23
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images23
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data23
CME-Flare Association and the Role of Reconnection in CME Acceleration23
Solar Filament Segmentation Based on Improved U-Nets22
Avalanching Together: A Model for Sympathetic Flaring22
The Mean Temperatures of CME-Related Dimming Masses21
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data20
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy19
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes19
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery19
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S19
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning19
Potential Field Source Surface and Non-linear Force-Free Field Extrapolation to Model Magnetic Field Structure for a Giant Solar Filament18
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations17
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)16
Linear Correlation Between Radial and Normal Component Fluctuations of the Interplanetary Magnetic Field16
Forecasting Solar Flares by Data Assimilation in Sandpile Models16
A Study on the Various Modes of Parallel Heat Conduction in the Coronal Loops of Small and Large Solar Flares Using Scaling Laws15
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology15
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution14
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD14
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 2414
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions13
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components13
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data13
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series13
An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data13
Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope13
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles13
An Efficient Method for Magnetic Field Extrapolation Based on a Family of Analytical Three-Dimensional Magnetohydrostatic Equilibria13
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma12
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts12
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions12
Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind12
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial11
Lifetime of Sunspots and Pores11
Predicting Solar Cycle 26 Using the Polar Flux as a Precursor, Spectral Analysis, and Machine Learning: Crossing a Gleissberg Minimum?11
Detections of Multi-Periodic Oscillations During a Circular Ribbon Flare11
Solar Flare Effects on the Earth’s Lower Ionosphere11
The Future of Solar Modelling: Requirements for a New Generation of Solar Models11
Deciphering Solar Magnetic Activity: 140 Years of the ‘Extended Solar Cycle’ – Mapping the Hale Cycle11
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope10
A Study of Variations in Correlation Between Rotation Residual and Meridional Velocity of Sunspot Groups10
The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles10
A Synchronized Two-Dimensional $\alpha $–$\Omega $ Model of the Solar Dynamo10
Structures of Various Types of Symmetry in the Solar Activity Cycle10
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
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions10
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability10
Corotating Interaction Regions during Solar Cycle 24: A Study on Characteristics and Geoeffectiveness10
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission10
Propagating Oscillations in the Lower Atmosphere Under Coronal Holes10
Sunspots Identification Through Mathematical Morphology10
Fabry-Pérot Interferometer Based Imaging Spectrometer for Fe I Line Observation and Line-of-Sight Velocity Measurement10
Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona9
Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms Using the uGMRT9
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique9
Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model9
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
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 Forecasts8
Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms ($\mathrm{Dst} \le -100$ nT) from 1932 to 20188
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
Correction to: On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis8
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)8
Adding Further Pieces to the Synchronization Puzzle: QBO, Bimodality, and Phase Jumps8
Improvements to the Empirical Solar Wind Forecast (ESWF) model8
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations8
The “SEP Clock”: A Discussion of First Proton Arrival Times in Wide-Spread Solar Energetic Particle Events8
Modelling Persistent Cycles in Solar Activity8
Heliolatitudinal Distribution and Hemispheric Asymmetry of Source Locations for Super Geomagnetic Storms (Dst ≤−250 nT) During Different Phases of Solar Cycles8
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19698
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 248
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.78
Tidally Synchronized Solar Dynamo: A Rebuttal8
Correction to: Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 247
Differential Rotation of Solar Filaments Early Observed by the OGAUC in the Period 1929 – 19417
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20217
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter7
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles7
Kinematic Study of Radio-Loud CMEs Associated with Solar Flares and DH Type-II Radio Emissions During Solar Cycles 23 and 247
Clarifying Physical Properties of Magnetic Fields in Sunspots7
Time Lag Between Cosmic-Ray and Solar Variability: Sunspot Numbers and Open Solar Magnetic Flux7
On the Magnetoacoustic Waves and Physical Conditions in Zebra Radio Sources7
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images7
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon7
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe7
HelioIndex: A Directory of Active Researchers in Solar and Heliospheric Physics7
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation7
Evaluating Pointing Strategies for Future Solar Flare Missions7
Correction to: Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances7
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes7
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos7
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis7
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence7
Meridional Movements of Individual Sunspots and Pores7
The Gondola for the Sunrise iii Balloon-Borne Solar Observatory6
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)6
Turbulence in Sources of Decimetric Flare Continua6
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
Segmentation of Coronal Features to Understand the Solar EUV and UV Irradiance Variability III. Inclusion and Analysis of Bright Points6
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)6
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 246
Sunspot Rotation in High- and Low-Flaring Active Regions6
Long-Term Variation of Helioseismic Far-Side Images and What Causes It6
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques6
Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field6
Probing Upflowing Regions in the Quiet Sun and Coronal Holes6
Solar-Cycle Variability Results from the Solar Radiation and Climate Experiment (SORCE) Mission6
Coronal Density Measurements Using Giant Radio Pulses of the Crab Pulsar at the Cycle 24/25 Minimum6
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle6
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations6
Solar Soft X-Ray Irradiance Variability, II: Temperature Variations of Coronal X-Ray Features6
Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns?6
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”6
An Enhanced ResNet Model for Solar Activity Classification with Dual-Passband CHASE Data6
The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 20246
A Study on the Transition-Range Spectral Index of the Solar Wind Turbulence in the Inner Heliosphere6
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
Multi-Wavelength Observations of Quasi-Periodic Pulsations in a Solar Flare6
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
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20236
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere6
Data-Driven Forecasting of Sunspot Cycles: Pros and Cons of a Hybrid Approach6
How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes6
Changing Methodologies in Solar Physics6
The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase5
Alfvén Pulse in a Chromospheric Magnetic Tube and Generation of the Super-Dreicer Electric Field5
Amplitudes of Solar Gravity Modes: A Review5
Noise in Maps of the Sun at Radio Wavelengths II: Solar Use Cases5
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
Improved Tomographic Reconstruction of 3D Global Coronal Density from STEREO/COR1 Observations5
Polarimetric Studies of a Fast Coronal Mass Ejection5
A Study on Correcting the Effect of Polarization Crosstalk in Full-Disk Solar Photospheric Magnetic Field Observations5
A Comparison of Sparse and Non-sparse Techniques for Electric-Field Inversion from Normal-Component Magnetograms5
A Stellar View of the Sun5
Ripples and Rush-to-the-Poles in the Photospheric Magnetic Field5
Precursory Signs of Large Forbush Decreases: The Criterion of Anisotropy5
Annual Variations in the Near-Earth Solar Wind5
Analysis of Galactic Cosmic Ray Anisotropy During the Time Period from 1996 to 20205
The Narrow Field Imager (NFI) for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)5
Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission5
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132835
Accuracy Analysis of the On-board Data Reduction Pipeline for the Polarimetric and Helioseismic Imager on the Solar Orbiter Mission5
Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 265
Dynamics of Explosive Events Observed by the Interface Region Imaging Spectrograph5
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations5
Properties of EUV Imaging Spectrometer (EIS) Slot Observations5
Reply to “Response to ‘Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators’ by R.J. Booth”5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Correction to: A Discussion of Implausible Total Solar-Irradiance Variations Since 17005
A New Global Nonlinear Force-Free Coronal Magnetic-Field Extrapolation Code Implemented on a Yin–Yang Grid5
A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI5
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis5
Synthetic Resonance and Thomson Scattering of a Chromospheric $\text{Ly}\alpha $ Profile Using the Bastille Day CME Model Corona: Part 15
On the Estimation of the SHARP Parameter MEANALP from AIA Images Using Deep Neural Networks5
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 255
Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption That Resulted in a Sustained Gamma Ray Emission Event5
An MHD Study of Large-Amplitude Oscillations in Solar Filaments5
Solar Irradiance Spectra from the Compact SOLSTICE (CSOL) Experiment: Instrument Design, FUV Calibration, Measurements, and Comparison of the 2018 Rocket Flight5
Intense Geomagnetically Induced Currents (GICs): Association with Solar and Geomagnetic Activities5
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter5
Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances5
Magnetic Field and Plasma Diagnostics for Solar Coronal Mass Ejections: A Case Study Using the Forward Modeling Approach4
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 Magne4
Long-Term Trend Analysis in the Solar Radiation and Climate Experiment (SORCE)/Spectral Irradiance Monitor (SIM)4
Similarities and Differences of SARs in Solar Cycle 244
The Sun’s Non-Potential Corona over Solar Cycle 244
Distributions of Mesoscale Periodic Structures in the Elemental and Ionic Composition of the Solar Wind4
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
Spectral Analysis of Rieger Periodicity Behaviour in O and Fe Galactic Cosmic Particles Observed by ACE in Solar Cycles 23 and 244
Nonlinear Propagating Slow Waves in Cooling Coronal Magnetic Loops4
Solar Low Energy X-ray Spectrometer (SoLEXS) on Board Aditya-L1 Mission4
Data Processing Pipeline of the SUTRI EUV Imager on the SATech-01 Satellite4
The Properties of Non-Potential Magnetic Field Parameters in a Super-Active Region with Complex Structures and Strong Solar Flares4
Solar-Filament Detection and Classification Based on Deep Learning4
Properties of Type-II Radio Bursts in Relation to Magnetic Complexity of the Solar Active Regions4
The Hazard of UV-Induced Oxidation to Solar-Viewing Spacecraft Optics4
Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection4
The Sun’s Large-Scale Flows I: Measurements of Differential Rotation & Torsional Oscillation4
On the Most Interesting Solar-Wind and Cosmic-Ray Events in February–April 20234
How Hot Can Small Solar Flares Get?4
Visible Emission Line Coronagraph (VELC) on Board Aditya-L14
Solar Rotation in the Period 1611 – 1631 Determined Using Observations of Christoph Scheiner4
Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager4
Systems Approach to Polarization Calibration for the Daniel K. Inouye Solar Telescope (DKIST)4
Data-Constrained Magnetohydrodynamics Simulation of a Confined X-Class Flare in NOAA Active Region 111664
Periodic Variation of Anomalous Cosmic Ray Oxygen During Solar Cycles 23 and 244
CATEcor: An Open Science, Shaded-Truss, Externally-Occulted Coronagraph4
First Hard X-Ray Imaging Results by Solar Orbiter STIX4
Hydrogen Ionization Inside the Sun4
Coronal Electric Currents and Kink Instability of Magnetic Flux Rope4
Detection of “Diffuse” Coronal He I 1083 During the April 8, 2024 Solar Eclipse: Evidence for Terrestrial Atmospheric Scattering Contribution4
Solar Active Regions Detection and Tracking Based on Deep Learning4
Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods4
The First Survey of Quiet Sun Features Observed in Hard X-Rays with NuSTAR4
Anticipating Solar Flares4
Forecasting Solar Cycle 25 with Physical Model-Validated Recurrent Neural Networks3
Sympathetic Quiet and Active Region Filament Eruptions3
Correction to: Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions3
Solar Radio Burst Prediction Based on a Multimodal Model3
SOLar-STellar Irradiance Comparison Experiment II (SOLSTICE II): End-of-Mission Validation of the SOLSTICE Technique3
Subsurface Horizontal Flows During Solar Cycles 24 and 25 with Large-Tile Ring-Diagram Analysis3
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
Exploring the Origin of Stealth Coronal Mass Ejections with Magnetofrictional Simulations3
Comparison of Polar Magnetic Fields Derived from MILOS and MERLIN Inversions with Hinode/SOT-SP Data3
Editorial Appreciation3
The Fibre Resolved OpticAl and Near-Ultraviolet Czerny–Turner Imaging Spectropolarimeter (francis)3
On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis3
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 Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME3
Forecasting the Dst Index with Temporal Convolutional Network and Integrated Gradients3
Statistical Analysis of Sunspot Area and Magnetic Flux on Solar Disc During 2011 – 20233
Wide-Field Image Restoration of G-Band and Ca ii K Images Containing Large and Complex Active Regions3
Reduced Microwave Brightness Temperature in a Sunspot Atmosphere Due to Open Magnetic Fields3
A New Solar Hard X-ray Image Reconstruction Algorithm for ASO-S/HXI Based on Deep Learning3
Solar Soft X-ray Irradiance Variability III: Magnetic Field Variations of Coronal X-ray Features3
Obituary: Tadashi Hirayama (1934 – 2025)3
Rudolf Wolf to Alfred Wolfer: The Transfer of the Reference Observer in the International Sunspot Number Series (1876–1893)3
Characteristics of Suprathermal Electrons in Small-Scale Magnetic Flux Ropes and Their Implications on the Magnetic Connection to the Sun3
Solar Flare Catalogue from 3 Years of Chandrayaan-2 XSM Observations3
The Solar Radiation and Climate Experiment (SORCE) Mission: Final Calibrations and Data Products3
On the Hierarchical Relationship Between Type-II Radio Bursts and the Associated Coronal Mass Ejections3
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
New Anisotropic Cosmic-Ray Enhancement (ACRE) Event on 5 November 2023 Due to Complex Heliospheric Conditions3
Temporal and Latitudinal Variation in Penumbra-Umbra Ratios of the Sunspots: Analyses of RGO, Kodaikanal and Debrecen Databases3
Ground-Level Enhancement of 8 June 2024 (GLE 75) Caused by Solar Energetic Particles3
Forecasting Medium-Term F10.7 Using the Deep-Learning Informer Model3
Improvements of the Longitudinal Magnetic Field Measurement from the Solar Magnetic Field Telescope at the Huairou Solar Observing Station3
Magnetic Imbalance at Supergranular Scale: A Driving Mechanism for Coronal Hole Formation3
Observation of Alfvén Waves in an ICME-HSS Interaction Region3
One Possible Reason for Switchback Formation3
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