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 2022-08-01 to 2026-08-01.)
ArticleCitations
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube101
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S78
Avalanching Together: A Model for Sympathetic Flaring50
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes31
Observations of Switchback Chains in a Twin-CME Event31
Accelerating Multiframe Blind Deconvolution via Deep Learning30
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2429
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 177729
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit24
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images24
The Mean Temperatures of CME-Related Dimming Masses24
Shock Signatures of the Successive Type-II Solar Radio Bursts at Meter Wavelength23
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data23
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data22
CME-Flare Association and the Role of Reconnection in CME Acceleration22
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200321
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”18
Analog-Based Forecasting of Solar Cycles Using Dynamic Time Warping and Residual Bootstrapping: Real-Time Application to Cycle 2517
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind17
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions17
On the Relation Between Upflow Velocities and Coronal Non-thermal Velocities as Measured by Hinode/EIS17
Potential Field Source Surface and Non-linear Force-Free Field Extrapolation to Model Magnetic Field Structure for a Giant Solar Filament16
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations16
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 2416
Linear Correlation Between Radial and Normal Component Fluctuations of the Interplanetary Magnetic Field15
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy15
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD15
Accelerated Electron Kinetics and Hard X-ray Pulsations in Solar Flares14
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles14
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components14
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology13
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning13
MHD Simulations of CME with Associated Prominence Eruption13
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions13
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution13
Editorial Appreciation13
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series12
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)12
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery12
Sharper than Ever: Do Modern Observations Pin down the Solar Radius to Converge on New Standards?12
Spatiotemporal Machine-Learning Detection of Coronal Mass Ejections in SOHO/LASCO C2 Images12
Forecasting Solar Flares by Data Assimilation in Sandpile Models12
The EUV Late-Phase: Statistical Results from 15 Years of Solar Dynamics Observatory Observations12
Polarimeter to Unify the Corona and Heliosphere (PUNCH)12
Prediction of Solar Activity Using Neutrosophic Fuzzy Time Series: A Study of Yearly and Monthly Hemispherical SSNs12
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial11
Lifetime of Sunspots and Pores11
Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope11
Predicting Solar Cycle 26 Using the Polar Flux as a Precursor, Spectral Analysis, and Machine Learning: Crossing a Gleissberg Minimum?11
Determination of 3He-Rich Periods Measured by the Suprathermal Ion Telescope on STEREO-A During Solar Cycle 2411
An Efficient Method for Magnetic Field Extrapolation Based on a Family of Analytical Three-Dimensional Magnetohydrostatic Equilibria11
Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind11
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma11
Polarity Reversal of the Polar Magnetic Fields in Solar Cycle 2511
Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries11
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data11
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts11
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions11
Structures of Various Types of Symmetry in the Solar Activity Cycle10
A Multi-Viewpoint CME Catalog Based on SoloHI Observed Events10
Multiscale Aspects of the Solar Indexes Mg II, F10.7 and Sunspot Number10
The Future of Solar Modelling: Requirements for a New Generation of Solar Models10
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 Corona10
The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: An Instrument for SUNRISE III10
The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles10
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope10
Citizen CATE 2024: Extending Totality During the 8 April 2024 Total Solar Eclipse with a Distributed Network of Community Participants9
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)9
Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms Using the uGMRT9
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19699
Unravelling Rieger and Quasi-Biennial Periodic Trends and Asymmetries in Coronal Mass Ejections Using Wavelet Analysis9
SSTrack: An Automatic Sunspot Identification and Tracking Algorithm to Support the Measurement of Sunspot Rotation9
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 D9
Sunspots Identification Through Mathematical Morphology9
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission9
Modeling Decadal and Centennial Solar UV Irradiance Changes9
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations9
Sources of a Stationary Type II Radio Burst on the Associated Coronal Mass Ejection Driven-Shocks9
Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model9
Application of a Neural Network for Identifying Erroneous Solar Images9
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability9
Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts9
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 Events9
A Synchronized Two-Dimensional $\alpha $–$\Omega $ Model of the Solar Dynamo9
Effective Hybrid Ensemble Deep-Learning Models for Century-Long Forecasting of Sunspot Solar Cycle from 2020-21108
Comparing Magnetic Field Distribution of Active Regions: Part 1 Methods of Mode Analysis8
Disambiguation of Cool and Hot Emission in SDO/AIA Channels and IRIS/Slit-Jaw Imager8
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images8
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence8
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20218
Meridional Movements of Individual Sunspots and Pores8
Adding Further Pieces to the Synchronization Puzzle: QBO, Bimodality, and Phase Jumps8
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)8
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 248
Flare Energetics, CME Launch and Heliospheric Propagation for the May 2024 Events, as Derived from Ensemble MHD Modelling8
Correction to: Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 248
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis8
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation8
Heliolatitudinal Distribution and Hemispheric Asymmetry of Source Locations for Super Geomagnetic Storms (Dst ≤−250 nT) During Different Phases of Solar Cycles8
Tidally Synchronized Solar Dynamo: A Rebuttal8
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique8
Improvements to the Empirical Solar Wind Forecast (ESWF) model8
HelioIndex: A Directory of Active Researchers in Solar and Heliospheric Physics8
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.78
Short and Intermediate Periodicities in Ca ii K Plage Areas as Seen in Kodaikanal Images for Individual Cycles from 14 to 227
Parametric Decay Instability as a Source of Turbulence in an Open Leakage Permitting Vertical Solar Coronal Domain7
Aditya-L1 - An Observatory Class Mission: Spacecraft, Mission, and Operations7
Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns?7
On Prediction of Solar Wind Speed Large-Scale Structures Using the Solar Full-Disk Multi-Layer Magnetograph - the New Chinese Facility Constructed for the International Meridian Circle Program7
Data-Driven Forecasting of Sunspot Cycles: Pros and Cons of a Hybrid Approach7
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes7
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles7
Advances in the Physics of the Sun and the Solar-Heliosphere Connection – Editorial7
Sunspot Rotation in High- and Low-Flaring Active Regions7
Changing Methodologies in Solar Physics7
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos7
Clarifying Physical Properties of Magnetic Fields in Sunspots7
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe7
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter7
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”7
An Enhanced ResNet Model for Solar Activity Classification with Dual-Passband CHASE Data7
Differential Rotation of Solar Filaments Early Observed by the OGAUC in the Period 1929 – 19417
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon7
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations6
Joint Inversion of Radionuclide Production Rate Data and Thermoremanent Magnetic Records over the Holocene6
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20236
A Study on the Transition-Range Spectral Index of the Solar Wind Turbulence in the Inner Heliosphere6
Quantifying Chromosphere Response to Flare Energy Release Using AIA Observations in 1600 Å and 304 Å Passbands6
Polarization Diagnostics Applied to Coronal Mass Ejections and the Background Solar Wind6
Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 266
How the Solar Dynamics Observatory Advanced Our Physical Understanding of the Sun6
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
Turbulence in Sources of Decimetric Flare Continua6
Hybrid ANN+PSO Technique for Accurate Short-Term F10.7 Index Forecasting6
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere6
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
The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 20246
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques6
The Role of Photospheric Magnetic Flux Diffusion in Initiation of Solar Eruptions6
The Sun as a Rosetta Stone for Understanding Star–Planet Interactions6
A Stellar View of the Sun6
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
Statistical Study of Intense Geomagnetic Storms and Their Solar Origins over the Period 1996 – 20256
Statistical Properties and Solar Cycle Distribution of Solar Proton Events Across Three Intensity Classes6
Three Decades of Global Oscillation Network Group (GONG): From Helioseismology to Magnetic Field and Space Weather (Invited Review)6
Solar Soft X-Ray Irradiance Variability, II: Temperature Variations of Coronal X-Ray Features6
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)6
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle6
Diagnosing Coronal Magnetic Fields with Slow Magnetoacoustic Waves: The Role of Isothermal Speeds6
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations6
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
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)6
Partial Null-Point Reconnection of an Eruptive Filament6
The Wide Field Imager (WFI) Instruments for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)6
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
Design and Implementation of a Multi-Element Solar Radio Interferometer at 1.42 GHz5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Nonlinear Propagating Slow Waves in Cooling Coronal Magnetic Loops5
On the Onset of the X1.3-Class Flare in NOAA Active Region 129755
A New Global Nonlinear Force-Free Coronal Magnetic-Field Extrapolation Code Implemented on a Yin–Yang Grid5
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 255
Amplitudes of Solar Gravity Modes: A Review5
A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI5
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter5
Accuracy Analysis of the On-board Data Reduction Pipeline for the Polarimetric and Helioseismic Imager on the Solar Orbiter Mission5
Improved Tomographic Reconstruction of 3D Global Coronal Density from STEREO/COR1 Observations5
Synthetic Resonance and Thomson Scattering of a Chromospheric $\text{Ly}\alpha $ Profile Using the Bastille Day CME Model Corona: Part 15
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
Correction to: A Discussion of Implausible Total Solar-Irradiance Variations Since 17005
A Statistical Study of $\delta $-Sunspots from Solar Cycle 23 to 255
Data Processing Pipeline of the SUTRI EUV Imager on the SATech-01 Satellite5
Neupert Effect: A Statistical Analysis of M and X-Class Flares During Cycle 245
Alfvén Pulse in a Chromospheric Magnetic Tube and Generation of the Super-Dreicer Electric Field5
Noise in Maps of the Sun at Radio Wavelengths II: Solar Use Cases5
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code5
Large-Scale Solar Magnetic Fields Observed with Full-Disk Telescopes at the Sayan and Baikal Observatories: Similarities, Differences, and Application to the Space-Weather Issues5
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132835
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 Deep-Learning Framework for Super Resolution Reconstruction of SOHO/MDI Magnetograms5
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
Observations of Flare Induced Doppler Shifts in the Si iii 1206 Å Line5
Brightenings AnD Polarity Inversion Tracking (BADPIT) Method for Studying Solar Active Region Evolution Before Major Solar Flares5
Annual Variations in the Near-Earth Solar Wind5
Machine Learning–Based Characterization of Solar p-Mode Frequency Shifts During Solar Cycle 255
Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission5
The Narrow Field Imager (NFI) for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)5
The Performance of a Blast Wave Model in Predicting Arrival Times of the Interplanetary Shocks from January 2013 to July 20235
The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy5
Ripples and Rush-to-the-Poles in the Photospheric Magnetic Field5
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