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 2021-05-01 to 2025-05-01.)
ArticleCitations
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200368
The Mean Temperatures of CME-Related Dimming Masses64
Spatial and Temporal Variations of 2 – 10 MeV nuc−1 He/H in Gradual Solar Energetic Particle Events48
Solar Filament Segmentation Based on Improved U-Nets35
Detection of Coronal Mass Ejections Using Unsupervised Deep Clustering32
Fabry–Pérot Interferometer-Based Tunable Narrow-Band Imager for Solar Chromospheric Observation: First Results31
Numerical Simulation of Longitudinal Oscillation of Filament Based on Smoothed Particle Hydrodynamics (SPH) Method30
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind30
Rate of Change of Large-Scale Solar-Wind Structure29
Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 2428
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit28
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube28
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S27
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 Acceleration24
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images24
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”24
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions22
Correction to: Kanzelhöhe Observatory: Instruments, Data Processing and Data Products22
Accelerating Multiframe Blind Deconvolution via Deep Learning22
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery21
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning21
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series21
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)20
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology20
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy20
A Study on the Various Modes of Parallel Heat Conduction in the Coronal Loops of Small and Large Solar Flares Using Scaling Laws20
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles18
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD18
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions17
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components17
North–South Asymmetry of Solar Meridional Circulation and Synchronization: Two Rings of Four Coupled Oscillators17
Forecasting Solar Flares by Data Assimilation in Sandpile Models17
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution17
Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 2416
Solar Rotation Multiples in Space-Weather Effects16
Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?16
The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations15
Thermal Trigger for Solar Flares II: Effect of the Guide Magnetic Field14
Improved Approach in the Coupling Function Between Primary and Ground Level Cosmic Ray Particles Based on Neutron Monitor Data14
Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope14
Predicting Solar Cycle 26 Using the Polar Flux as a Precursor, Spectral Analysis, and Machine Learning: Crossing a Gleissberg Minimum?14
Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind14
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts13
Deciphering Solar Magnetic Activity: 140 Years of the ‘Extended Solar Cycle’ – Mapping the Hale Cycle13
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial13
Two Classes of Eruptive Events During Solar Minimum13
Corotating Interaction Regions during Solar Cycle 24: A Study on Characteristics and Geoeffectiveness13
Solar Flare Effects on the Earth’s Lower Ionosphere13
An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data12
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma12
Lifetime of Sunspots and Pores12
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data12
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions12
A Study of Variations in Correlation Between Rotation Residual and Meridional Velocity of Sunspot Groups11
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission11
Marshall Grazing Incidence X-ray Spectrometer Slitjaw Imager Implementation and Performance11
Detections of Multi-Periodic Oscillations During a Circular Ribbon Flare11
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 D11
Two-Stage Evolution of an Extended C-Class Eruptive Flaring Activity from Sigmoid Active Region NOAA 12734: SDO and Udaipur-CALLISTO Observations11
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)11
Structures of Various Types of Symmetry in the Solar Activity Cycle11
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope11
Propagating Oscillations in the Lower Atmosphere Under Coronal Holes11
Sunspots Identification Through Mathematical Morphology11
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
Fabry-Pérot Interferometer Based Imaging Spectrometer for Fe I Line Observation and Line-of-Sight Velocity Measurement10
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability10
Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona10
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions9
Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model9
Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms ($\mathrm{Dst} \le -100$ nT) from 1932 to 20189
Radio Interferometric Observations of the Sun Using Commercial Dish TV Antennas9
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19699
Multiscale Aspects of the Solar Indexes Mg II, F10.7 and Sunspot Number9
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique9
Scaling Features of Diurnal Variation of Galactic Cosmic Rays9
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
Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts9
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)9
Tidally Synchronized Solar Dynamo: A Rebuttal8
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)8
Time Lag Between Cosmic-Ray and Solar Variability: Sunspot Numbers and Open Solar Magnetic Flux8
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations8
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
Correction to: On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis8
Modelling Persistent Cycles in Solar Activity8
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
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis7
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos7
Data-Driven Forecasting of Sunspot Cycles: Pros and Cons of a Hybrid Approach7
Clarifying Physical Properties of Magnetic Fields in Sunspots7
Differential Rotation of Solar Filaments Early Observed by the OGAUC in the Period 1929 – 19417
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes7
Kinematic Study of Radio-Loud CMEs Associated with Solar Flares and DH Type-II Radio Emissions During Solar Cycles 23 and 247
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation7
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon7
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
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20217
Evaluating Pointing Strategies for Future Solar Flare Missions7
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence7
Correction to: Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances7
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe7
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere6
How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes6
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter6
Segmentation of Coronal Features to Understand the Solar EUV and UV Irradiance Variability III. Inclusion and Analysis of Bright Points6
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20236
Probing Upflowing Regions in the Quiet Sun and Coronal Holes6
On the Nature of the Kink MHD Waves in Flowing and Twisted Coronal Flux Tubes6
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle6
Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 246
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
Separating the aa-index into Solar and Hale Cycle Related Components Using Principal Component Analysis6
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
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
Turbulence in Sources of Decimetric Flare Continua6
Solar Wind Discontinuity Interaction with the Bow Shock: Current Density Growth and Dawn-Dusk Asymmetry6
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques6
Reply to Comment on “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field”6
Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns?6
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles6
Sunspot Rotation in High- and Low-Flaring Active Regions6
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations6
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
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
Multi-Wavelength Observations of Quasi-Periodic Pulsations in a Solar Flare6
Long-Term Variation of Helioseismic Far-Side Images and What Causes It6
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations5
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter5
Resonant Instability of Kink Oscillations in Magnetic Flux Tubes with Siphon Flow5
High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis5
Annual Variations in the Near-Earth Solar Wind5
The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase5
Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission5
Polarimetric Studies of a Fast Coronal Mass Ejection5
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
Accuracy Analysis of the On-board Data Reduction Pipeline for the Polarimetric and Helioseismic Imager on the Solar Orbiter Mission5
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)5
Solar-Cycle Variability Results from the Solar Radiation and Climate Experiment (SORCE) Mission5
On the Estimation of the SHARP Parameter MEANALP from AIA Images Using Deep Neural Networks5
Extreme Space-Weather Events and the Solar Cycle5
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 255
An MHD Study of Large-Amplitude Oscillations in Solar Filaments5
Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods5
Analysis of Galactic Cosmic Ray Anisotropy During the Time Period from 1996 to 20205
Amplitudes of Solar Gravity Modes: A Review5
Ripples and Rush-to-the-Poles in the Photospheric Magnetic Field5
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
Reply to “Response to ‘Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators’ by R.J. Booth”5
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
Properties of EUV Imaging Spectrometer (EIS) Slot Observations5
A Study on Correcting the Effect of Polarization Crosstalk in Full-Disk Solar Photospheric Magnetic Field Observations5
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132835
A Study on the Transition-Range Spectral Index of the Solar Wind Turbulence in the Inner Heliosphere5
Latitude Variations in Primary and Secondary Polar Crown Polarity Inversion Lines and Polar Coronal Hole Boundaries over Five Solar Cycles5
A Comparison of Sparse and Non-sparse Techniques for Electric-Field Inversion from Normal-Component Magnetograms5
A New Global Nonlinear Force-Free Coronal Magnetic-Field Extrapolation Code Implemented on a Yin–Yang Grid5
Anticipating Solar Flares5
Solar Cycle Dependence of ICME Composition5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
Kodaikanal Solar Observatory Radio Spectrograph5
A Stellar View of the Sun5
Dynamics of Explosive Events Observed by the Interface Region Imaging Spectrograph5
0.08779501914978