Solar Physics

Papers
(The TQCC of Solar Physics is 5. 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 2021-08-01 to 2025-08-01.)
ArticleCitations
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200377
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events56
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) Method38
Rate of Change of Large-Scale Solar-Wind Structure34
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube33
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit31
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S29
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2427
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 177726
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”26
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions25
Accelerating Multiframe Blind Deconvolution via Deep Learning25
Correction to: Kanzelhöhe Observatory: Instruments, Data Processing and Data Products24
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes24
CME-Flare Association and the Role of Reconnection in CME Acceleration23
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind23
Avalanching Together: A Model for Sympathetic Flaring22
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images22
Solar Filament Segmentation Based on Improved U-Nets21
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning20
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data20
The Mean Temperatures of CME-Related Dimming Masses20
Potential Field Source Surface and Non-linear Force-Free Field Extrapolation to Model Magnetic Field Structure for a Giant Solar Filament19
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy19
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery19
Forecasting Solar Flares by Data Assimilation in Sandpile Models18
Linear Correlation Between Radial and Normal Component Fluctuations of the Interplanetary Magnetic Field18
A Study on the Various Modes of Parallel Heat Conduction in the Coronal Loops of Small and Large Solar Flares Using Scaling Laws18
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations18
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology18
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD17
Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?16
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution16
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions15
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 2415
Solar Rotation Multiples in Space-Weather Effects15
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components14
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)14
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles14
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 Efficient Method for Magnetic Field Extrapolation Based on a Family of Analytical Three-Dimensional Magnetohydrostatic Equilibria13
Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope13
An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data13
Predicting Solar Cycle 26 Using the Polar Flux as a Precursor, Spectral Analysis, and Machine Learning: Crossing a Gleissberg Minimum?12
Lifetime of Sunspots and Pores12
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts12
Deciphering Solar Magnetic Activity: 140 Years of the ‘Extended Solar Cycle’ – Mapping the Hale Cycle12
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions12
Solar Flare Effects on the Earth’s Lower Ionosphere12
Detections of Multi-Periodic Oscillations During a Circular Ribbon Flare12
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma12
Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind11
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission11
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial11
Structures of Various Types of Symmetry in the Solar Activity Cycle11
The Future of Solar Modelling: Requirements for a New Generation of Solar Models11
Corotating Interaction Regions during Solar Cycle 24: A Study on Characteristics and Geoeffectiveness11
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
Multiscale Aspects of the Solar Indexes Mg II, F10.7 and Sunspot Number10
Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model10
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability10
Propagating Oscillations in the Lower Atmosphere Under Coronal Holes10
A Study of Variations in Correlation Between Rotation Residual and Meridional Velocity of Sunspot Groups10
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)10
Sunspots Identification Through Mathematical Morphology10
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions10
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope10
The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles10
Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona10
A Synchronized Two-Dimensional $\alpha $–$\Omega $ Model of the Solar Dynamo10
Fabry-Pérot Interferometer Based Imaging Spectrometer for Fe I Line Observation and Line-of-Sight Velocity Measurement10
Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms Using the uGMRT9
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations9
Scaling Features of Diurnal Variation of Galactic Cosmic Rays9
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.79
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique9
Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts9
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 249
A Multi-Viewpoint CME Catalog Based on SoloHI Observed Events9
Active Region Contributions to the Solar Wind over Multiple Solar Cycles9
Correction to: On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis9
The “SEP Clock”: A Discussion of First Proton Arrival Times in Wide-Spread Solar Energetic Particle Events8
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)8
On the Magnetoacoustic Waves and Physical Conditions in Zebra Radio Sources8
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
Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms ($\mathrm{Dst} \le -100$ nT) from 1932 to 20188
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19698
Tidally Synchronized Solar Dynamo: A Rebuttal8
Correction to: Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances8
Time Lag Between Cosmic-Ray and Solar Variability: Sunspot Numbers and Open Solar Magnetic Flux8
Improvements to the Empirical Solar Wind Forecast (ESWF) model8
Modelling Persistent Cycles in Solar Activity8
Correction to: Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 248
Radio Interferometric Observations of the Sun Using Commercial Dish TV Antennas8
Differential Rotation of Solar Filaments Early Observed by the OGAUC in the Period 1929 – 19418
Kinematic Study of Radio-Loud CMEs Associated with Solar Flares and DH Type-II Radio Emissions During Solar Cycles 23 and 247
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe7
Evaluating Pointing Strategies for Future Solar Flare Missions7
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes7
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon7
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence7
Solar Soft X-Ray Irradiance Variability, II: Temperature Variations of Coronal X-Ray Features7
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
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles7
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20217
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis7
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter7
Meridional Movements of Individual Sunspots and Pores7
Sunspot Rotation in High- and Low-Flaring Active Regions7
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation7
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos7
Clarifying Physical Properties of Magnetic Fields in Sunspots7
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images7
HelioIndex: A Directory of Active Researchers in Solar and Heliospheric Physics7
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere7
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”7
Dynamics of Explosive Events Observed by the Interface Region Imaging Spectrograph6
On the Estimation of the SHARP Parameter MEANALP from AIA Images Using Deep Neural Networks6
Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field6
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
Long-Term Variation of Helioseismic Far-Side Images and What Causes It6
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)6
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20236
Changing Methodologies in Solar Physics6
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
A Study on Correcting the Effect of Polarization Crosstalk in Full-Disk Solar Photospheric Magnetic Field Observations6
Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 266
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
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
Segmentation of Coronal Features to Understand the Solar EUV and UV Irradiance Variability III. Inclusion and Analysis of Bright Points6
An Enhanced ResNet Model for Solar Activity Classification with Dual-Passband CHASE Data6
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 246
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
On the Nature of the Kink MHD Waves in Flowing and Twisted Coronal Flux Tubes6
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations6
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 256
The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 20246
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 Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques6
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle6
How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes6
Turbulence in Sources of Decimetric Flare Continua6
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations6
Correction to: A Discussion of Implausible Total Solar-Irradiance Variations Since 17005
Intense Geomagnetically Induced Currents (GICs): Association with Solar and Geomagnetic Activities5
Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods5
Latitude Variations in Primary and Secondary Polar Crown Polarity Inversion Lines and Polar Coronal Hole Boundaries over Five Solar Cycles5
Reply to “Response to ‘Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators’ by R.J. Booth”5
Amplitudes of Solar Gravity Modes: A Review5
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
Noise in Maps of the Sun at Radio Wavelengths II: Solar Use Cases5
Solar Irradiance Spectra from the Compact SOLSTICE (CSOL) Experiment: Instrument Design, FUV Calibration, Measurements, and Comparison of the 2018 Rocket Flight5
High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis5
Accuracy Analysis of the On-board Data Reduction Pipeline for the Polarimetric and Helioseismic Imager on the Solar Orbiter Mission5
Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances5
An MHD Study of Large-Amplitude Oscillations in Solar Filaments5
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
A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI5
Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission5
Analysis of Galactic Cosmic Ray Anisotropy During the Time Period from 1996 to 20205
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132835
Polarimetric Studies of a Fast Coronal Mass Ejection5
A Stellar View of the Sun5
Kodaikanal Solar Observatory Radio Spectrograph5
Alfvén Pulse in a Chromospheric Magnetic Tube and Generation of the Super-Dreicer Electric Field5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Annual Variations in the Near-Earth Solar Wind5
A Comparison of Sparse and Non-sparse Techniques for Electric-Field Inversion from Normal-Component Magnetograms5
The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase5
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
The Narrow Field Imager (NFI) for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)5
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter5
Properties of EUV Imaging Spectrometer (EIS) Slot Observations5
Improved Tomographic Reconstruction of 3D Global Coronal Density from STEREO/COR1 Observations5
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