Space Weather-The International Journal of Research and Applications

Papers
(The TQCC of Space Weather-The International Journal of Research and Applications is 7. 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 2021-06-01 to 2025-06-01.)
ArticleCitations
71
A Space Weather Approach for Quasi‐Real‐Time Assessment of Satellite Orbital Decay During Geomagnetic Storms Based on Two‐Line Element Sets67
Picturing Global Substorm Dynamics in the Magnetotail Using Low‐Altitude ELFIN Measurements and Data Mining‐Based Magnetic Field Reconstructions64
PreMevE‐MEO: Predicting Ultra‐Relativistic Electrons Using Observations From GPS Satellites63
Prediction of Energetic Electrons in the Inner Radiation Belt and Slot Region With a Double‐Layer LSTM Neural Network Model62
Issue Information54
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Toward GIC Forecasting: Statistical Downscaling of the Geomagnetic Field to Improve Geoelectric Field Forecasts43
SRF2—A Short‐Term (1–24)h foF2 Prediction Method42
Ensemble Modeling of Radiation Belt Electron Acceleration by Chorus Waves: Dependence on Key Input Parameters36
Low Altitude Tailing Es (LATTE): Analysis of Sporadic‐E Layer Height at Different Latitudes of Middle and Low Region34
Substorm Induced Nighttime Plasma Flow Pulsations Observed by ROCSAT‐1 at Topside Ionosphere33
Linkage of Equatorial Ionization Anomaly With the Day‐To‐Day Occurrence of Postsunset Irregularities and Scintillation in Low‐Latitude Region Around 110°E31
Storm‐Time Characteristics of Ionospheric Model (MSAP) Based on Multi‐Algorithm Fusion31
Credit Where Credit Is Due: Data and Software in the Space Weather Community30
Evaluating Auroral Forecasts Against Satellite Observations30
Forecasting Ionospheric foF2 Using Bidirectional LSTM and Attention Mechanism30
Ground GNSS Station Selection to Generate the Global Ionosphere Maps Using the Information Content29
Predicting Geomagnetic Activity Cycles28
First Observations of a Geomagnetic Superstorm With a Sub‐L1 Monitor28
Observations of Geomagnetic Crochet at High‐Latitudes Due To X1.5 Class Solar Flare on 3 July 202128
Influence of Tectonic and Geological Structure on GIC in Southern South Island, New Zealand27
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Issue Information26
A 3D Empirical Model of Electron Density Based on CSES Radio Occultation Measurements25
The Need for a Sub‐L1 Space Weather Research Mission: Current Knowledge Gaps on Coronal Mass Ejections25
Machine Learning for Predicting the Bz Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections25
A Bayesian Inference‐Based Empirical Model for Scintillation Indices for High‐Latitude25
Double Superposed Epoch Analysis of Geomagnetic Storms and Corresponding Solar Wind and IMF in Solar Cycles 23 and 2425
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Statistical Characterization of GITM Thermospheric Horizontal Winds in Comparison to GOCE Estimations24
OSPREI: A Coupled Approach to Modeling CME‐Driven Space Weather With Automatically Generated, User‐Friendly Outputs24
Improved and Interpretable Solar Flare Predictions With Spatial and Topological Features of the Polarity Inversion Line Masked Magnetograms24
A Framework to Estimate Local Atmospheric Densities With Reduced Drag‐Coefficient Biases23
Development of a Regional F‐Region Critical Frequency Model for Southern Africa23
Daytime F Region Echoes at Equatorial Ionization Anomaly Crest During Geomagnetic Quiet Period: Observations From Multi‐Instruments23
SWOL2023: Report of Space Weather Observations Throughout Latinoamerica: Filling the Southern Gaps23
The Response of Ionospheric Currents to External Drivers Investigated Using a Neural Network‐Based Model22
A Substorm‐Dependent Negative Limit of Non‐Eclipse Surface Charging of a Chinese Geosynchronous Satellite22
A Real‐Time Prediction System of the Intensity of Solar Energetic Proton Events Based on a Solution of the Diffusion Equation21
Nowcasting Solar EUV Irradiance With Photospheric Magnetic Fields and the Mg II Index21
Modeling the Impact of Geomagnetically Induced Currents on Electrified Railway Signaling Systems in the United Kingdom21
Space Weather Effects on Transportation Systems: A Review of Current Understanding and Future Outlook20
Modeling Pipe to Soil Potentials From Geomagnetic Storms in Gas Pipelines in New Zealand20
Solar Tide‐like Signatures in the Ionospheric Total Electron Content During the 2018 Sudden Stratospheric Warming Event20
Attention‐Based Machine Vision Models and Techniques for Solar Wind Speed Forecasting Using Solar EUV Images20
GOLD Observations of Equatorial Plasma Bubbles Reaching Mid‐Latitudes During the 23 April 2023 Geomagnetic Storm19
Magnetic Signatures of Ionospheric Disturbance Dynamo for CME and HSSWs Generated Storms18
Prediction Interval of Interface Regions: Machine Learning Nowcasting Approach18
Multi‐Site Transfer Function Approach for Real‐Time Modeling of the Ground Electric Field Induced by Laterally‐Nonuniform Ionospheric Source18
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Very High Energy Solar Energetic Particle Events and Ground Level Enhancement Events: Forecasting and Alerts18
Ionospheric Turbulence: A Challenge for GPS Loss of Lock Understanding17
3D Modeling of Geomagnetically Induced Currents in Sweden—Validation and Extreme Event Analysis17
Forecasting the Remaining Duration of an Ongoing Solar Flare17
72‐Hour Time Series Forecasting of Hourly Relativistic Electron Fluxes at Geostationary Orbit by Deep Learning17
Drag‐Based CME Modeling With Heliospheric Images Incorporating Frontal Deformation: ELEvoHI 2.017
Bayesian Inference and Global Sensitivity Analysis for Ambient Solar Wind Prediction16
Meeting Report: International Magnetosphere Coupling IV (IMC‐IV) Workshop GFZ‐Potsdam, Germany, 2–7 June 202416
Ionospheric Nowcasting Over Italy Through Data Assimilation: A Synergy Between IRI UP and IONORING16
Nighttime Geomagnetic Response to Jumps of Solar Wind Dynamic Pressure: A Possible Cause of Québec Blackout in March 198916
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The Error of Global Ionospheric Map‐TEC During Equatorial Plasma Bubble Event in the High Solar Activity Year16
Forecasting of the Geomagnetic Activity for the Next 3 Days Utilizing Neural Networks Based on Parameters Related to Large‐Scale Structures of the Solar Corona16
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Potential of Regional Ionosphere Prediction Using a Long Short‐Term Memory Deep‐Learning Algorithm Specialized for Geomagnetic Storm Period15
Time‐Lagged Effects of Ionospheric Response to Severe Geomagnetic Storms on GNSS Kinematic Precise Point Positioning15
A New Model for Nowcasting the Aviation Radiation Environment With Comparisons to In Situ Measurements During GLEs15
Investigation of the Contribution of Five Broadcast Ionospheric Models (GPSK, NTCMG, NEQG, BDGIM, and BDSK) and IRTG to GNSS Positioning During Different Solar Activities in Solar Cycle 2515
Machine‐Learning Research in the Space Weather Journal: Prospects, Scope, and Limitations15
Equatorial Plasma Bubble Detection Using Vertical TEC From Altimetry Satellite15
Unveiling the Space Weather During the Starlink Satellites Destruction Event on 4 February 202215
Static and Dynamic Model Calibration for Upper Thermosphere Determination15
Assessing the Effects of a Minor CIR‐HSS Geomagnetic Storm on the Brazilian Low‐Latitude Ionosphere: Ground and Space‐Based Observations15
The Impact of Sudden Commencements on Ground Magnetic Field Variability: Immediate and Delayed Consequences15
Global Sensitivity Analysis of Nitric Oxide‐Related Chemical Reaction Rates in the Global Ionosphere Thermosphere Model14
Assessment of Space Weather Impacts on New Zealand Power Transformers Using Dissolved Gas Analysis14
Response of the Thermosphere‐Ionosphere System to an X‐Class Solar Flare: 30 March 2022 Case Study14
An Empirical Relationship Between Coronal Density and Solar Wind Velocity in the Middle Corona With Applications to Space Weather14
Issue Information14
Measurements of Cosmic Rays by a Mini‐Neutron Monitor at Neumayer III From 2014 to 201714
Data Assimilation of Ion Drift Measurements for Estimation of Ionospheric Plasma Drivers13
Prediction of Proton Pressure in the Outer Part of the Inner Magnetosphere Using Machine Learning13
Decent Estimate of CME Arrival Time From a Data‐Assimilated Ensemble in the Alfvén Wave Solar Atmosphere Model (DECADE‐AWSoM)13
Turning Noise Into Data: Characterization of the Van Allen Radiation Belt Using SDO Spikes Data13
Development of the Ionospheric E‐Region Prompt Radio Occultation Based Electron Density (E‐PROBED) Model13
Case Studies on the Day‐to‐Day Variability in the Occurrence of Post‐Sunset Equatorial Spread F13
New Detailed Modeling of GICs in the Spanish Power Transmission Grid13
High‐Latitude Electrodynamics Specified in SAMI3 Using AMPERE Field‐Aligned Currents13
Investigating the Effects of Ionospheric Scintillation on Multi‐Frequency BDS‐2/BDS‐3 Signals at Low Latitudes12
Investigation on Horizontal and Vertical Traveling Ionospheric Disturbances Propagation in Global‐Scale Using GNSS and Multi‐LEO Satellites12
The First Ground‐Level Enhancement of Solar Cycle 25 as Seen by the High‐Energy Particle Detector (HEPD‐01) on Board the CSES‐01 Satellite12
Long‐Term Support Is Needed for Crucial Ground‐Based Sensor Networks12
Even‐Order Harmonic Distortion Observations During Multiple Geomagnetic Disturbances: Investigation From New Zealand12
Issue Information12
Estimation Model of Global Ionospheric Irregularities: An Artificial Intelligence Approach12
What to Do When the F10.7 Goes Out?12
Magnetopause Standoff Position Changes and Geosynchronous Orbit Crossings: Models and Observations12
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Modeling Meteorological Effects on Cosmic Ray Muons Utilizing Multivariate Analysis11
An Examination of SuperDARN Backscatter Modes Using Machine Learning Guided by Ray‐Tracing11
Estimates of Spherical Satellite Drag Coefficients in the Upper Thermosphere During Different Geomagnetic Conditions11
Validation of Ionospheric Specifications During Geomagnetic Storms: TEC and foF2 During the 2013 March Storm Event‐II11
Climatological Statistics of Extreme Geomagnetic Fluctuations With Periods From 1 s to 60 min11
Thermospheric Temperature and Density Variability During 3–4 February 2022 Minor Geomagnetic Storm11
New Space Companies Meet a “Normal” Solar Maximum11
Using a Differential Magnetometer Technique to Measure Geomagnetically Induced Currents: An Augmented Approach11
A Comparison of Auroral Oval Proxies With the Boundaries of the Auroral Electrojets11
Solar Flare X‐Ray Impacts on Long Subionospheric VLF Paths11
Observations From NOAA's Newest Solar Proton Sensor11
Implications of Using Spheroidal “Cone Model” CMEs in Solar‐Wind Models11
Analysis of Large Geomagnetically Induced Currents During the 7–8 September 2017 Storm: Geoelectric Field Mapping11
Physics‐Based Approach to Thermospheric Density Estimation Using CubeSat GPS Data11
Prediction of the SYM‐H Index Using a Bayesian Deep Learning Method With Uncertainty Quantification11
Deep Learning for Global Ionospheric TEC Forecasting: Different Approaches and Validation11
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Modeling Ionospheric TEC Using Gradient Boosting Based and Stacking Machine Learning Techniques11
Implementing an Operational Cloud‐Based Now‐ and Forecasting System for Space Weather Ground Effects in the UK11
Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array11
Calibration of Swarm Plasma Densities Overestimation Using Neural Networks11
An Empirical Model of the Equatorial Electron Pitch Angle Distributions in Earth's Outer Radiation Belt10
Dayside Magnetic Depression Following Interplanetary Shock Arrivals During the February 1958 and July 1959 Superstorms10
Quantitative Assessment of GOES 8–15 > ${ >} $0.6 and > ${ >} $4 MeV Radiation Belt Electron Fluxes10
Sensitivity of Model Estimates of CME Propagation and Arrival Time to Inner Boundary Conditions10
Automatic Detection and Classification of Spread‐F From Ionosonde at Hainan With Image‐Based Deep Learning Method10
New Index to Characterize Ionospheric Irregularity Distribution10
Reduced Order Probabilistic Emulation for Physics‐Based Thermosphere Models10
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Storm‐Time Ring Current Plasma Pressure Prediction Based on the Multi‐Output Convolutional Neural Network Model10
Machine‐Learned HASDM Thermospheric Mass Density Model With Uncertainty Quantification10
Partially Erupted Prominence Material as a Diagnostic of Coronal Mass Ejection Trajectory10
Influences of Solar Wind Parameters on Energetic Electron Fluxes at Geosynchronous Orbit Revealed by the Deep SHAP Method10
Resolving Moving Heliospheric Structures Using Interplanetary Scintillation Observations With the Murchison Widefield Array10
Comparative Analysis of Higher‐Order Ionospheric Delay on PPP Long‐Term Coordinate Time Series and Residual Modeling Using Horizontal Gradients and RINEX Data10
Interpretable Machine Learning for Thermospheric Mass Density Modeling Using GRACE/GRACE‐FO Satellite Data10
Solar Wind Speed Prediction With Two‐Dimensional Attention Mechanism10
Examining the Economic Costs of the 2003 Halloween Storm Effects on the North Hemisphere Aviation Using Flight Data in 201910
Characterization of Radiation Exposure at Aviation Flight Altitudes Using the Nowcast of Aerospace Ionizing Radiation System (NAIRAS)10
An Examination of Geomagnetic Induction in Submarine Cables10
Interpretable Machine Learning to Forecast SEP Events for Solar Cycle 239
Estimation of the Solar Wind Extreme Events9
The Impact of Lower Atmosphere Forecast Uncertainties on WACCM‐X Prediction of Ionosphere‐Thermosphere System During Geomagnetic Storms9
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Radio Absorption in the Nightside Ionosphere of Mars During Solar Energetic Particle Events9
Different Response of the Ionospheric TEC and EEJ to Ultra‐Fast Kelvin Waves in the Mesosphere and Lower Thermosphere9
Measurements and Modeling of the Responses of VLF Transmitter Signals to X‐Class Solar Flares at the Great Wall Station in Antarctica9
Qualitative and Quantitative Assessment of the SET HASDM Database9
CMEs and SEPs During November–December 2020: A Challenge for Real‐Time Space Weather Forecasting9
Enhanced Radiation Levels at Aviation Altitudes and Their Relationship to Plasma Waves in the Inner Magnetosphere9
2024 Decadal Survey for Space and Solar Physics: Space Weather Inputs9
TEC Map Completion Through a Deep Learning Model: SNP‐GAN9
Space Weather Into the 2030s: The 2024 Solar and Space Physics Decadal Survey9
Issue Information9
Extreme Event Statistics in Dst, SYM‐H, and SMR Geomagnetic Indices9
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On the Geoelectric Field Response to the SSC of the May 2024 Super Storm Over Europe9
Quantifying Uncertainties in the Quiet‐Time Ionosphere‐Thermosphere Using WAM‐IPE9
Dynamical Complexity Transitions During High‐Intensity Long Duration Continuous Auroral Activities (HILDCAA) Events: Feature Analysis Based on Neural Network Entropy9
Response of the Ionospheric TEC to SSW and Associated Geomagnetic Storm Over the American Low Latitudinal Sector9
Global Observations of the Short‐Term Disturbances in the Geomagnetic Field and Induced Currents During the Supersubstorms Events of Solar Cycle 249
The Mother's Day Geomagnetic Storm on 10 May 2024: Aurora Observations and Low Latitude Space Weather Effects in Mexico9
Impact of Ionospheric Scintillations on GNSS Availability and Precise Positioning9
Improving Solar Wind Forecasting Using Data Assimilation9
Correcting Projection Effects in CMEs Using GCS‐Based Large Statistics of Multi‐Viewpoint Observations9
Quantification of Representation Error in the Neutral Winds and Ion Drifts Using Data Assimilation9
The Frequency‐Domain Characterization of Cosmic Ray Intensity Variations Before Forbush Decreases Associated With Geomagnetic Storms9
Super‐Intense Geomagnetic Storm on 10–11 May 2024: Possible Mechanisms and Impacts9
Numerical Modeling and GNSS Observations of Ionospheric Depletions Due To a Small‐Lift Launch Vehicle9
Over 20‐Year Global Magnetohydrodynamic Simulation of Earth's Magnetosphere8
Comparative Analysis of TPA‐LSTM and Transformer Models for Forecasting GEO Radiation Belt Electron Fluxes8
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Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks8
Mapping a Magnetic Superstorm: March 1989 Geoelectric Hazards and Impacts on United States Power Systems8
Solar Wind and Magnetospheric Conditions for Satellite Anomalies Attributed to Shallow Internal Charging8
Specifying High Altitude Electrons Using Low‐Altitude LEO Systems: Updates to the SHELLS Model8
CME Evolution in the Structured Heliosphere and Effects at Earth and Mars During Solar Minimum8
The Effect of Midnight Temperature Maximum Winds on Post‐Midnight Equatorial Spread F8
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Geomagnetically Induced Currents at Middle Latitudes: 1. Quiet‐Time Variability8
Development and Validation of Precipitation Enhanced Densities for the Empirical Canadian High Arctic Ionospheric Model8
Predicting Equatorial Spread F at JICAMARCA Sector Via Supervised Machine Learning8
Observations of Unusual Postsunrise Interhemispheric Geomagnetic Conjugate Super Plasma Depletions at Midlatitudes During the Recovery Phase of the November 2003 Superstorm8
Thank You to Our 2021 Peer Reviewers8
Responses of the African and American Equatorial Ionization Anomaly (EIA) to 2014 Arctic SSW Events8
On the Growth and Evolution of Nocturnal Ionospheric Irregularities Using HF Radar Observations Along With Digisonde and GNSS Data Over Trivandrum, India8
Influence of Solar Wind High‐Speed Streams on the Brazilian Low‐Latitude Ionosphere During the Descending Phase of Solar Cycle 248
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New Findings From Explainable SYM‐H Forecasting Using Gradient Boosting Machines8
Forecasting the Probability of Large Rates of Change of the Geomagnetic Field in the UK: Timescales, Horizons, and Thresholds8
Specifying Satellite Drag Through Coupled Thermosphere‐Ionosphere Data Assimilation of Radio Occultation Electron Density Profiles8
Spatial and Temporal Confinement of the Ionospheric Responses During the St. Patrick's Day Storm of March 20158
Impacts of Auroral Precipitation on HF Propagation: A Hypothetical Over‐the‐Horizon Radar Case Study7
PyIRI: Whole‐Globe Approach to the International Reference Ionosphere Modeling Implemented in Python7
Interhemispheric Asymmetry in the High‐Latitude Neutral Density Variations During the 13–14 March 2022 Storm7
Issue Information7
MEMPSEP‐I. Forecasting the Probability of Solar Energetic Particle Event Occurrence Using a Multivariate Ensemble of Convolutional Neural Networks7
The Growth of Ring Current/SYM‐H Under Northward IMF Bz Conditions Present During the 21–22 January 2005 Geomagnetic Storm7
A Parametric Study of Performance of Two Solar Wind Velocity Forecasting Models During 2006–20117
Modeling TEC Irregularities in the Arctic Ionosphere Using Empirical Orthogonal Function Method7
The Impact of Space Radiation on Brains of Future Martian and Lunar Explorers7
3‐D Ionospheric Imaging Over the South American Region With a New TEC‐Based Ionospheric Data Assimilation System (TIDAS‐SA)7
Thank You to Our Peer Reviewers in 20247
A Method to Mitigate the Effects of Strong Geomagnetic Storm on GNSS Precise Point Positioning7
Solar Wind—Magnetosphere Coupling Functions: Pitfalls, Limitations, and Applications7
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PyIRTAM: A New Module of PyIRI for IRTAM Coefficients7
Improving Precise Orbit Determination of LEO Satellites Using Enhanced Solar Radiation Pressure Modeling7
The Short‐Time Prediction of Thermospheric Mass Density Based on Ensemble‐Transfer Learning7
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Forward‐Looking Study of Solar Maximum Impact in 2025: Effects of Satellite Navigation Failure on Aviation Network Operation in the Greater Bay Area, China7
Statistical Study on the Effect of Meridional Neutral Wind on the Occurrence of Post‐Sunset Equatorial Ionospheric Irregularities7
Understanding Strong Neutral Vertical Winds and Ionospheric Responses to the 2015 St. Patrick's Day Storm Using TIEGCM Driven by Data‐Assimilated Aurora and Electric Fields7
Predicting Equatorial Ionospheric Convective Instability Using Machine Learning7
MHD‐Test Particles Simulations of Moderate CME and CIR‐Driven Geomagnetic Storms at Solar Minimum7
Ionospheric Response to the M‐ and X‐Class Solar Flares of 28 October 2021 Over the African Sector7
Issue Information7
TIE‐GCM ROPE ‐ Dimensionality Reduction: Part I7
SIR‐HUXt—A Particle Filter Data Assimilation Scheme for CME Time‐Elongation Profiles7
A Transfer Learning Method to Generate Synthetic Synoptic Magnetograms7
A Prediction Model of Relativistic Electrons at Geostationary Orbit Using the EMD‐LSTM Network and Geomagnetic Indices7
Probabilistic Solar Proxy Forecasting With Neural Network Ensembles7
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