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 2022-07-01 to 2026-07-01.)
ArticleCitations
Nonlinear Generation of Fluting Perturbations by Kink Mode in a Twisted Magnetic Tube100
The Solar Aspect System of the Hard X-ray Imager Onboard ASO-S77
Avalanching Together: A Model for Sympathetic Flaring49
The Solar Origin of an Intense Geomagnetic Storm on 1 December 2023: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes38
Observations of Switchback Chains in a Twin-CME Event32
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 177728
Photometric Comparison of Metis and LASCO-C2 Polarized Brightness Images27
Rate of Change of Large-Scale Solar-Wind Structure27
On the Possibility of Measuring Solar Flattening from Photometry Measurements Taken during Solar Eclipses Seen from the Earth’s Surface or Earth Orbit23
Shock Signatures of the Successive Type-II Solar Radio Bursts at Meter Wavelength22
The Mean Temperatures of CME-Related Dimming Masses22
Data-Driven Reconstruction of a Low-Order Dynamo Model from Sunspot Data21
Analog-Based Forecasting of Solar Cycles Using Dynamic Time Warping and Residual Bootstrapping: Real-Time Application to Cycle 2520
Differential Rotation of Long-Lived Sunspot Groups in Solar Cycles 22 – 24 Determined by Watukosek Solar Observatory Data20
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 200319
CME-Flare Association and the Role of Reconnection in CME Acceleration18
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
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”16
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
Potential Field Source Surface and Non-linear Force-Free Field Extrapolation to Model Magnetic Field Structure for a Giant Solar Filament15
Multiwavelength Observations of a Breakout Jet at an Active Region Periphery14
Cloud Removal of Full-Disk Solar H$\alpha $ Images Based on RPix2PixHD14
Forecasting Solar Flares by Data Assimilation in Sandpile Models14
Arecibo Multifrequency IPS Observations: Solar-Wind Density Turbulence Scale Sizes and Their Anisotropy14
Accelerated Electron Kinetics and Hard X-ray Pulsations in Solar Flares14
HMI Ring-Diagram Analysis: Effects of Tracking, Noise, and Resolution13
Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles13
Magnetic Evolution of an Active Region Producing Successive Flares and Confined Eruptions13
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components13
Prediction of Geoeffective CMEs Using SOHO Images and Deep Learning13
Editorial Appreciation13
Stacked 1D Convolutional LSTM (sConvLSTM1D) Model for Effective Prediction of Sunspot Time Series12
Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology12
MHD Simulations of CME with Associated Prominence Eruption12
Polarimeter to Unify the Corona and Heliosphere (PUNCH)12
The EUV Late-Phase: Statistical Results from 15 Years of Solar Dynamics Observatory Observations12
The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)12
Sharper than Ever: Do Modern Observations Pin down the Solar Radius to Converge on New Standards?11
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma11
Predicting Solar Cycle 26 Using the Polar Flux as a Precursor, Spectral Analysis, and Machine Learning: Crossing a Gleissberg Minimum?11
A SART-Based Iterative Inversion Methodology to Infer the Solar Rotation Rate from Global Helioseismic Data11
Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries11
Determination of 3He-Rich Periods Measured by the Suprathermal Ion Telescope on STEREO-A During Solar Cycle 2411
Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope11
Solar X-Band Imaging with the Arecibo 12-m Telescope: The Brightness Temperature and Magnetic Field of Active Regions11
Lifetime of Sunspots and Pores11
The Future of Solar Modelling: Requirements for a New Generation of Solar Models11
Structures of Various Types of Symmetry in the Solar Activity Cycle11
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts11
Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind11
An Efficient Method for Magnetic Field Extrapolation Based on a Family of Analytical Three-Dimensional Magnetohydrostatic Equilibria11
Polarity Reversal of the Polar Magnetic Fields in Solar Cycle 2511
Magnetohydrodynamic (MHD) Waves and Oscillations in the Sun’s Corona and MHD Coronal Seismology: Editorial11
A Multi-Viewpoint CME Catalog Based on SoloHI Observed Events10
The State of the White-Light Corona over the Minimum and Ascending Phases of Solar Cycle 25 – Comparison with Past Cycles10
Citizen CATE 2024: Extending Totality During the 8 April 2024 Total Solar Eclipse with a Distributed Network of Community Participants10
Fabry-Pérot Interferometer Based Imaging Spectrometer for Fe I Line Observation and Line-of-Sight Velocity Measurement10
Modeling Decadal and Centennial Solar UV Irradiance Changes10
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
Sunspots Identification Through Mathematical Morphology10
Multiscale Aspects of the Solar Indexes Mg II, F10.7 and Sunspot Number10
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
Relationships Between Physical Parameters of Umbral Dots Measured for 12 Sunspot Umbras with the Goode Solar Telescope10
Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms Using the uGMRT9
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)9
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.79
Adding Further Pieces to the Synchronization Puzzle: QBO, Bimodality, and Phase Jumps9
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 249
The “SEP Clock”: A Discussion of First Proton Arrival Times in Wide-Spread Solar Energetic Particle Events9
Heliolatitudinal Distribution and Hemispheric Asymmetry of Source Locations for Super Geomagnetic Storms (Dst ≤−250 nT) During Different Phases of Solar Cycles9
Application of a Neural Network for Identifying Erroneous Solar Images9
Predicting Maximum Amplitude and Rise Time of Solar Cycle 25 Using Modified Geomagnetic Precursor Technique9
Tidally Synchronized Solar Dynamo: A Rebuttal9
Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts9
Improvements to the Empirical Solar Wind Forecast (ESWF) model9
Two New Sub-GLEs Found in Data of Neutron Monitors at South Pole and Vostok: On 09 June 1968 and 27 February 19699
Correction to: On the Strength and Duration of Solar Cycle 25: A Novel Quantile-Based Superposed-Epoch Analysis9
Acoustic Waves in a High-Temperature Plasma II. Damping and Instability9
Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model9
SSTrack: An Automatic Sunspot Identification and Tracking Algorithm to Support the Measurement of Sunspot Rotation9
Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations9
Plasma-Analyzer Package for Aditya (PAPA) on Board the Indian Aditya-L1 Mission9
Flare Energetics, CME Launch and Heliospheric Propagation for the May 2024 Events, as Derived from Ensemble MHD Modelling9
Unravelling Rieger and Quasi-Biennial Periodic Trends and Asymmetries in Coronal Mass Ejections Using Wavelet Analysis9
Sources of a Stationary Type II Radio Burst on the Associated Coronal Mass Ejection Driven-Shocks9
Meridional Movements of Individual Sunspots and Pores8
Effective Hybrid Ensemble Deep-Learning Models for Century-Long Forecasting of Sunspot Solar Cycle from 2020-21108
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images8
Hemispheric Asymmetry in the Sunspot Cycle as a Nonextensive Phenomenon8
High-Resolution Observation of Blowout Jets Regulated by Sunspot Rotation8
Parametric Decay Instability as a Source of Turbulence in an Open Leakage Permitting Vertical Solar Coronal Domain8
HelioIndex: A Directory of Active Researchers in Solar and Heliospheric Physics8
A Study of the Possible Mechanism of the Ground Level Enhancement on 28 October 20218
Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS)8
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
Average Subsurface Flows of Active and Quiet Regions with Large-Tile Ring-Diagram Analysis8
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter8
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe8
Disambiguation of Cool and Hot Emission in SDO/AIA Channels and IRIS/Slit-Jaw Imager8
Comparing Magnetic Field Distribution of Active Regions: Part 1 Methods of Mode Analysis8
Correction to: Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 248
Clarifying Physical Properties of Magnetic Fields in Sunspots8
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence8
Solar Poloidal Magnetic Field Generation Rate from Observations and Mean-Field Dynamos8
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Solar Limb Flare on February 5, 20237
Temporal and Periodic Analysis of Penumbra–Umbra Ratio for the Last Four Solar Cycles7
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
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
Three Decades of Global Oscillation Network Group (GONG): From Helioseismology to Magnetic Field and Space Weather (Invited Review)7
Data-Driven Forecasting of Sunspot Cycles: Pros and Cons of a Hybrid Approach7
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
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)7
Solar Flare Forecasting Based on Magnetogram Sequences Learning with Multiscale Vision Transformers and Data Augmentation Techniques7
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle7
Hybrid ANN+PSO Technique for Accurate Short-Term F10.7 Index Forecasting7
Short and Intermediate Periodicities in Ca ii K Plage Areas as Seen in Kodaikanal Images for Individual Cycles from 14 to 227
Sunspot Rotation in High- and Low-Flaring Active Regions7
Changing Methodologies in Solar Physics7
Photospheric Velocities Measured at Mt. Wilson Show Rotational and Poleward Velocity Deviations Compose the Torsional Oscillations7
Non-reflective Propagation of Kink Waves in Magnetic-Flux Tubes in the Solar Atmosphere7
Statistical Properties and Solar Cycle Distribution of Solar Proton Events Across Three Intensity Classes7
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
High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis6
The Role of Photospheric Magnetic Flux Diffusion in Initiation of Solar Eruptions6
Properties of EUV Imaging Spectrometer (EIS) Slot Observations6
Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption That Resulted in a Sustained Gamma Ray Emission Event6
Partial Null-Point Reconnection of an Eruptive Filament6
A Study on the Transition-Range Spectral Index of the Solar Wind Turbulence in the Inner Heliosphere6
Turbulence in Sources of Decimetric Flare Continua6
Statistical Study of Intense Geomagnetic Storms and Their Solar Origins over the Period 1996 – 20256
Hybrid-Ensemble Deep-Learning Models to Enhance the Sunspot Prediction and Forecasting of Solar Cycle 266
Neupert Effect: A Statistical Analysis of M and X-Class Flares During Cycle 246
A Statistical Study of $\delta $-Sunspots from Solar Cycle 23 to 256
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
Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field6
The Gondola for the Sunrise iii Balloon-Borne Solar Observatory6
The Sun as a Rosetta Stone for Understanding Star–Planet Interactions6
Diagnosing Coronal Magnetic Fields with Slow Magnetoacoustic Waves: The Role of Isothermal Speeds6
The Multifaceted M1.7 GOES-class Flare Event of 21 April 2023 in AR132836
Machine Learning–Based Characterization of Solar p-Mode Frequency Shifts During Solar Cycle 256
A Stellar View of the Sun6
Seismology of Curved Coronal Loops Using Multiperiodic Kink Oscillations6
How the Solar Dynamics Observatory Advanced Our Physical Understanding of the Sun6
The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 20246
Photospheric Stereoscopy: Direct Estimation of Solar Surface-Height Variations6
Correction to: The Solar Ultra-Violet Imaging Telescope (SUIT) Onboard Intelligence for Flare Observations6
The Magnetic-Field Calibration of the Full-Disk Magnetograph Onboard the Advanced Space Based Solar Observatory (ASO-S/FMG)6
Polarization Diagnostics Applied to Coronal Mass Ejections and the Background Solar Wind6
Three-Dimensional Reconstruction of Coronal Features: A Python Tool for Geometric Triangulation5
Correction to: A Discussion of Implausible Total Solar-Irradiance Variations Since 17005
Ripples and Rush-to-the-Poles in the Photospheric Magnetic Field5
Nonlinear Propagating Slow Waves in Cooling Coronal Magnetic Loops5
Solar Irradiance Spectra from the Compact SOLSTICE (CSOL) Experiment: Instrument Design, FUV Calibration, Measurements, and Comparison of the 2018 Rocket Flight5
Eruption-Related Ultraviolet Irradiance Enhancements Associated with Flares5
A Deep-Learning Framework for Super Resolution Reconstruction of SOHO/MDI Magnetograms5
The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy5
The Performance of a Blast Wave Model in Predicting Arrival Times of the Interplanetary Shocks from January 2013 to July 20235
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
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
Sloshing Oscillations in Hot Coronal Loops Associated with M-Class Flares5
Observations of Flare Induced Doppler Shifts in the Si iii 1206 Å Line5
Comment on: “Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field” by G. Verbanac and M. Bandić5
Data Processing Pipeline of the SUTRI EUV Imager on the SATech-01 Satellite5
The Coronal Flattening Index at the 20 April 2023 Total Solar Eclipse and the Prediction of Solar Cycle 255
Alfvén Pulse in a Chromospheric Magnetic Tube and Generation of the Super-Dreicer Electric Field5
Polarimetric Studies of a Fast Coronal Mass Ejection5
Amplitudes of Solar Gravity Modes: A Review5
Models of Collisionless Quasineutral Solar Wind Current Sheets5
A New Global Nonlinear Force-Free Coronal Magnetic-Field Extrapolation Code Implemented on a Yin–Yang Grid5
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
Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods5
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
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations5
Annual Variations in the Near-Earth Solar Wind5
Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter5
Design and Implementation of a Multi-Element Solar Radio Interferometer at 1.42 GHz5
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
On the Onset of the X1.3-Class Flare in NOAA Active Region 129755
A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI5
Spectroscopic He i 1083 nm Prominence Eruption Observations in the Middle Corona with MLSO/UCoMP4
Detection of “Diffuse” Coronal He I 1083 During the April 8, 2024 Solar Eclipse: Evidence for Terrestrial Atmospheric Scattering Contribution4
Correction to: Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods4
The Sun’s Large-Scale Flows I: Measurements of Differential Rotation & Torsional Oscillation4
Solar Active Regions Detection and Tracking Based on Deep Learning4
Solar Soft X-ray Irradiance Variability III: Magnetic Field Variations of Coronal X-ray Features4
Obituary: Tadashi Hirayama (1934 – 2025)4
On the Most Interesting Solar-Wind and Cosmic-Ray Events in February–April 20234
Solar Activity During the Peak of Solar Cycle 25 Captured by SiC UV Dosimeter Onboard EOS-084
The Hazard of UV-Induced Oxidation to Solar-Viewing Spacecraft Optics4
Properties of Type-II Radio Bursts in Relation to Magnetic Complexity of the Solar Active Regions4
Systems Approach to Polarization Calibration for the Daniel K. Inouye Solar Telescope (DKIST)4
Reconstruction of Carrington Rotation Means of Open Solar Flux over the Past 154 Years4
Analysis of Galactic Cosmic Ray Anisotropy During the Time Period from 1996 to 20204
The Sun’s Non-Potential Corona over Solar Cycle 244
Solar Rotation in the Period 1611 – 1631 Determined Using Observations of Christoph Scheiner4
The Eruption of 22 April 2021 as Observed by Solar Orbiter: Continuous Magnetic Reconnection and Heating After the Impulsive Phase4
The First Survey of Quiet Sun Features Observed in Hard X-Rays with NuSTAR4
Distributions of Mesoscale Periodic Structures in the Elemental and Ionic Composition of the Solar Wind4
Periodicity Variation in Solar UV Radiation (115 – 300 nm) During 2004 – 20194
Multiwavelength Observations of a Partial Filament Eruption on 13 June 20114
Similarities and Differences of SARs in Solar Cycle 244
Coronal Electric Currents and Kink Instability of Magnetic Flux Rope4
Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection4
How Hot Can Small Solar Flares Get?4
Periodic Variation of Anomalous Cosmic Ray Oxygen During Solar Cycles 23 and 244
Solar-Filament Detection and Classification Based on Deep Learning4
First Hard X-Ray Imaging Results by Solar Orbiter STIX4
Magnetic Reconnection at a Hyperbolic Flux Tube Associated with a Confined Flare in NOAA Active Region 122684
The Properties of Non-Potential Magnetic Field Parameters in a Super-Active Region with Complex Structures and Strong Solar Flares4
Magnetic Field and Plasma Diagnostics for Solar Coronal Mass Ejections: A Case Study Using the Forward Modeling Approach4
Precursory Signs of Large Forbush Decreases: The Criterion of Anisotropy4
Hydrogen Ionization Inside the Sun4
On the Penumbra-to-Umbra Ratio from 1660 to 16764
A Possible Connection between the de Vries Cycle and the Solar Dynamo4
Visible Emission Line Coronagraph (VELC) on Board Aditya-L14
Anticipating Solar Flares4
Data-Constrained Magnetohydrodynamics Simulation of a Confined X-Class Flare in NOAA Active Region 111664
Solar Low Energy X-ray Spectrometer (SoLEXS) on Board Aditya-L1 Mission4
CATEcor: An Open Science, Shaded-Truss, Externally-Occulted Coronagraph4
Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager4
Quasi-Separatrix Layers and Three-Dimensional Magnetic Reconnection: Theory and Observations of Solar Flares (Invited Review)4
Forecasting the Dst Index with Temporal Convolutional Network and Integrated Gradients3
New Anisotropic Cosmic-Ray Enhancement (ACRE) Event on 5 November 2023 Due to Complex Heliospheric Conditions3
Localization of the Gamma-Ray Emission Region in the 1 September 2014 Behind-the-Limb Solar Flare According to the Fermi/LAT Data3
Solar Orbiter’s 2024 Major Flare Campaigns: An Overview3
Comparison of Relative Magnetic Helicity Flux Calculation Results Based on the Line-of-Sight Magnetograms of ASO-S/FMG and SDO/HMI3
On the Formation of Collisionless Plasmoid Instability in Particle-in-Cell Simulations of the Solar Corona3
DETACH: Detection and Tracking Algorithm for Coronal Holes3
Correction to: Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions3
Solar Flare Catalogue from 3 Years of Chandrayaan-2 XSM Observations3
Visualization of High Dynamic Range Solar Imagery and the Radial Histogram Equalizing Filter3
Forecasting Solar Cycle 25 with Physical Model-Validated Recurrent Neural Networks3
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME3
Deep Learning-Enabled Prediction of Geoeffective CMEs Using SOHO and SDO Observations3
Solar Radio Burst Prediction Based on a Multimodal Model3
1.845860004425