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 2022-05-01 to 2026-05-01.)
ArticleCitations
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube96
Numerical Simulation of Longitudinal Oscillation of Filament Based on Smoothed Particle Hydrodynamics (SPH) Method72
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S47
Avalanching Together: A Model for Sympathetic Flaring37
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes32
Observations of Switchback Chains in a Twin-CME Event30
Accelerating Multiframe Blind Deconvolution via Deep Learning29
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2426
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions26
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”24
Bošković’s Spherical Trigonometric Solution for Determining the Axis and Rate of Solar Rotation by Observing Sunspots in 177724
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data21
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data20
Fabry–Pérot Interferometer-Based Tunable Narrow-Band Imager for Solar Chromospheric Observation: First Results20
Rate of Change of Large-Scale Solar-Wind Structure19
Shock Signatures of the Successive Type-II Solar Radio Bursts at Meter Wavelength18
The Mean Temperatures of CME-Related Dimming Masses18
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit18
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events17
CME-Flare Association and the Role of Reconnection in CME Acceleration16
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images16
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind16
Polarimeter to Unify the Corona and Heliosphere (PUNCH)15
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200315
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology15
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 2415
Linear Correlation Between Radial and Normal Component Fluctuations of the Interplanetary Magnetic Field14
Potential Field Source Surface and Non-linear Force-Free Field Extrapolation to Model Magnetic Field Structure for a Giant Solar Filament14
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations14
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy14
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery13
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)13
Forecasting Solar Flares by Data Assimilation in Sandpile Models13
MHD Simulations of CME with Associated Prominence Eruption12
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning12
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles12
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution12
Accelerated Electron Kinetics and Hard X-ray Pulsations in Solar Flares12
Editorial Appreciation12
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD12
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions12
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
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
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma11
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series11
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions11
The Future of Solar Modelling: Requirements for a New Generation of Solar Models11
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts11
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components11
Multiscale Aspects of the Solar Indexes Mg II, F10.7 and Sunspot Number10
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data10
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission10
The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles10
Lifetime of Sunspots and Pores10
Fabry-Pérot Interferometer Based Imaging Spectrometer for Fe I Line Observation and Line-of-Sight Velocity Measurement10
A Multi-Viewpoint CME Catalog Based on SoloHI Observed Events10
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial10
Structures of Various Types of Symmetry in the Solar Activity Cycle10
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)9
Sunspots Identification Through Mathematical Morphology9
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
Adding Further Pieces to the Synchronization Puzzle: QBO, Bimodality, and Phase Jumps9
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19699
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 249
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions9
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope9
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
Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms Using the uGMRT9
Citizen CATE 2024: Extending Totality During the 8 April 2024 Total Solar Eclipse with a Distributed Network of Community Participants9
Sources of a Stationary Type II Radio Burst on the Associated Coronal Mass Ejection Driven-Shocks9
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique9
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations9
Unravelling Rieger and Quasi-Biennial Periodic Trends and Asymmetries in Coronal Mass Ejections Using Wavelet Analysis9
Application of a Neural Network for Identifying Erroneous Solar Images9
Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona9
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability9
Modeling Decadal and Centennial Solar UV Irradiance Changes9
Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts9
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)9
Heliolatitudinal Distribution and Hemispheric Asymmetry of Source Locations for Super Geomagnetic Storms (Dst ≤−250 nT) During Different Phases of Solar Cycles9
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.79
Correction to: Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances8
Kinematic Study of Radio-Loud CMEs Associated with Solar Flares and DH Type-II Radio Emissions During Solar Cycles 23 and 248
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20218
Effective Hybrid Ensemble Deep-Learning Models for Century-Long Forecasting of Sunspot Solar Cycle from 2020-21108
Correction to: On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis8
Correction to: Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 248
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos8
Short and Intermediate Periodicities in Ca ii K Plage Areas as Seen in Kodaikanal Images for Individual Cycles from 14 to 228
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis8
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe8
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images8
Flare Energetics, CME Launch and Heliospheric Propagation for the May 2024 Events, as Derived from Ensemble MHD Modelling8
Tidally Synchronized Solar Dynamo: A Rebuttal8
Clarifying Physical Properties of Magnetic Fields in Sunspots8
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon8
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles8
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence8
Meridional Movements of Individual Sunspots and Pores8
Improvements to the Empirical Solar Wind Forecast (ESWF) model8
The “SEP Clock”: A Discussion of First Proton Arrival Times in Wide-Spread Solar Energetic Particle Events8
HelioIndex: A Directory of Active Researchers in Solar and Heliospheric Physics8
Differential Rotation of Solar Filaments Early Observed by the OGAUC in the Period 1929 – 19418
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes8
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation8
Joint Inversion of Radionuclide Production Rate Data and Thermoremanent Magnetic Records over the Holocene7
Solar Soft X-Ray Irradiance Variability, II: Temperature Variations of Coronal X-Ray Features7
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle7
Aditya-L1 - An Observatory Class Mission: Spacecraft, Mission, and Operations7
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”7
Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns?7
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere7
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)7
Statistical Properties and Solar Cycle Distribution of Solar Proton Events Across Three Intensity Classes7
Changing Methodologies in Solar Physics7
Data-Driven Forecasting of Sunspot Cycles: Pros and Cons of a Hybrid Approach7
Three Decades of Global Oscillation Network Group (GONG): From Helioseismology to Magnetic Field and Space Weather (Invited Review)7
An Enhanced ResNet Model for Solar Activity Classification with Dual-Passband CHASE Data7
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations7
Behaviour of 27-Day and 13.5-Day Periodicities in Galactic Cosmic Particles as Observed by Spacecraft and Neutron Monitors During Different Solar Polarity Cycles7
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20237
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter7
Sunspot Rotation in High- and Low-Flaring Active Regions7
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 247
A Study on the Transition-Range Spectral Index of the Solar Wind Turbulence in the Inner Heliosphere6
Turbulence in Sources of Decimetric Flare Continua6
Hybrid ANN+PSO Technique for Accurate Short-Term F10.7 Index Forecasting6
Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 266
Polarization Diagnostics Applied to Coronal Mass Ejections and the Background Solar Wind6
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132836
Properties of EUV Imaging Spectrometer (EIS) Slot Observations6
A Stellar View of the Sun6
Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field6
Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption That Resulted in a Sustained Gamma Ray Emission Event6
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
Partial Null-Point Reconnection of an Eruptive Filament6
The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 20246
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter6
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations6
Dynamics of Explosive Events Observed by the Interface Region Imaging Spectrograph6
Quantifying Chromosphere Response to Flare Energy Release Using AIA Observations in 1600 Å and 304 Å Passbands6
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques6
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
A Statistical Study of $\delta $-Sunspots from Solar Cycle 23 to 256
The Role of Photospheric Magnetic Flux Diffusion in Initiation of Solar Eruptions6
Diagnosing Coronal Magnetic Fields with Slow Magnetoacoustic Waves: The Role of Isothermal Speeds6
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 255
The Performance of a Blast Wave Model in Predicting Arrival Times of the Interplanetary Shocks from January 2013 to July 20235
Amplitudes of Solar Gravity Modes: A Review5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission5
Synthetic Resonance and Thomson Scattering of a Chromospheric $\text{Ly}\alpha $ Profile Using the Bastille Day CME Model Corona: Part 15
Guided Waves Along a Density Interface in Partially Ionised Solar Plasmas5
Neupert Effect: A Statistical Analysis of M and X-Class Flares During Cycle 245
Data Processing Pipeline of the SUTRI EUV Imager on the SATech-01 Satellite5
Ripples and Rush-to-the-Poles in the Photospheric Magnetic Field5
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code5
Polarimetric Studies of a Fast Coronal Mass Ejection5
Design and Implementation of a Multi-Element Solar Radio Interferometer at 1.42 GHz5
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
Systems Approach to Polarization Calibration for the Daniel K. Inouye Solar Telescope (DKIST)5
Machine Learning–Based Characterization of Solar p-Mode Frequency Shifts During Solar Cycle 255
Analysis of Galactic Cosmic Ray Anisotropy During the Time Period from 1996 to 20205
A Deep-Learning Framework for Super Resolution Reconstruction of SOHO/MDI Magnetograms5
Precursory Signs of Large Forbush Decreases: The Criterion of Anisotropy5
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI5
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
On the Onset of the X1.3-Class Flare in NOAA Active Region 129755
Solar Irradiance Spectra from the Compact SOLSTICE (CSOL) Experiment: Instrument Design, FUV Calibration, Measurements, and Comparison of the 2018 Rocket Flight5
The Narrow Field Imager (NFI) for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)5
Models of Collisionless Quasineutral Solar Wind Current Sheets5
Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods5
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
Nonlinear Propagating Slow Waves in Cooling Coronal Magnetic Loops5
Alfvén Pulse in a Chromospheric Magnetic Tube and Generation of the Super-Dreicer Electric Field5
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
A New Global Nonlinear Force-Free Coronal Magnetic-Field Extrapolation Code Implemented on a Yin–Yang Grid5
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