Journal of Space Weather and Space Climate

Papers
(The median citation count of Journal of Space Weather and Space Climate is 3. 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 2020-11-01 to 2024-11-01.)
ArticleCitations
What sustained multi-disciplinary research can achieve: The space weather modeling framework49
Accuracy assessment of the quiet-time ionospheric F2 peak parameters as derived from COSMIC-2 multi-GNSS radio occultation measurements38
The Interplanetary and Magnetospheric causes of Geomagnetically Induced Currents (GICs) > 10 A in the Mäntsälä Finland Pipeline: 1999 through 201937
The flare likelihood and region eruption forecasting (FLARECAST) project: flare forecasting in the big data & machine learning era31
Changes in the Total Solar Irradiance and climatic effects30
Graphical evidence for the solar coronal structure during the Maunder minimum: comparative study of the total eclipse drawings in 1706 and 171528
Sensing the ionosphere with the Spire radio occultation constellation25
Timelines as a tool for learning about space weather storms25
Thermosphere modeling capabilities assessment: geomagnetic storms21
Unexpected space weather causing the reentry of 38 Starlink satellites in February 202221
The Dalton Minimum and John Dalton’s Auroral Observations21
The operational and research DTM-2020 thermosphere models20
Solar Energetic Particle Event occurrence prediction using Solar Flare Soft X-ray measurements and Machine Learning20
Is the F10.7cm – Sunspot Number relation linear and stable?19
Unseasonal super ionospheric plasma bubble and scintillations seeded by the 2022 Tonga Volcano Eruption related perturbations19
Gas-surface interactions modelling influence on satellite aerodynamics and thermosphere mass density18
The Solar Activity Monitor Network – SAMNet17
Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect16
Geolectric field measurement, modelling and validation during geomagnetic storms in the UK15
ORFEES – a radio spectrograph for the study of solar radio bursts and space weather applications15
Geomagnetically induced currents during the 07–08 September 2017 disturbed period: a global perspective14
Global equivalent slab thickness model of the Earth’s ionosphere14
A note on the sunspot and prominence records made by Angelo Secchi during the period 1871–187514
Space Weather research in the Digital Age and across the full data lifecycle: Introduction to the Topical Issue13
A new climatological electron density model for supporting space weather services13
The Polar Cap (PC) index combination, PCC: relations to solar wind properties and global magnetic disturbances13
New thermosphere neutral mass density and crosswind datasets from CHAMP, GRACE, and GRACE-FO13
Plasmasphere and topside ionosphere reconstruction using METOP satellite data during geomagnetic storms13
Multi-instrument detection in Europe of ionospheric disturbances caused by the 15 January 2022 eruption of the Hunga volcano13
SunCET: The Sun Coronal Ejection Tracker Concept12
Evaluating the relationship between strong geomagnetic storms and electric grid failures in Poland using the geoelectric field as a GIC proxy12
Long-term studies of photospheric magnetic fields on the Sun12
MITO: a new directional muon telescope10
Occurrence rate and duration of space weather impacts on high-frequency radio communication used by aviation10
Timing of the solar wind propagation delay between L1 and Earth based on machine learning10
Reconstruction of the Parker spiral with the Reverse In situ data and MHD APproach – RIMAP10
Analytical and empirical modelling of the origin and heliospheric propagation of coronal mass ejections, and space weather applications10
An integrated data-driven solar wind – CME numerical framework for space weather forecasting9
The implications of ionospheric disturbances for precise GNSS positioning in Greenland9
Lensing from small-scale travelling ionospheric disturbances observed using LOFAR9
On a limitation of Zeeman polarimetry and imperfect instrumentation in representing solar magnetic fields with weaker polarization signal9
Modeling of ionospheric scintillation8
An inner boundary condition for solar wind models based on coronal density8
Geomagnetic field shielding over the last one hundred thousand years7
The probabilistic solar particle event forecasting (PROSPER) model7
Operational Dst index prediction model based on combination of artificial neural network and empirical model7
Prediction of the amplitude of solar cycle 25 using polar faculae observations7
The Great Aurora of 4 February 1872 observed by Angelo Secchi in Rome7
Uncertainty quantification of the DTM2020 thermosphere model7
Ionospheric plasma structuring in relation to auroral particle precipitation7
GNSS positioning error forecasting in the Arctic: ROTI and Precise Point Positioning error forecasting from solar wind measurements6
Growin: Modeling ionospheric instability growth rates6
Visualizing sporadic E using aeronautical navigation signals at VHF frequencies6
The relevance of local magnetic records when using extreme space weather events as benchmarks5
Combining Swarm Langmuir probe observations, LEO-POD-based and ground-based GNSS receivers and ionosondes for prompt detection of ionospheric earthquake and tsunami signatures: case study of 2015 Chil5
Observational evidence of thermospheric wind and composition changes and the resulting ionospheric disturbances in the European sector during extreme geomagnetic storms5
Auroral zone over the last 3000 years5
The refractive and diffractive contributions to GPS signal scintillation at high latitudes during the geomagnetic storm on 7–8 September 20175
Everyday space weather5
Responding trends of ionosphericF2-layer to weaker geomagnetic activities5
OMEP-EOR: A MeV proton flux specification model for electric orbit raising missions4
Geomagnetic activity recurrences for predicting the amplitude and shape of solar cycle n. 254
Inner radiation belt simulations of the proton flux response in the South Atlantic Anomaly during the Geomagnetic Storm of 15 May 20054
Semi-supervised classification of lower-ionospheric perturbations using GNSS radio occultation observations from Spire Global’s Cubesat Constellation4
Exploring possibilities for solar irradiance prediction from solar photosphere images using recurrent neural networks4
Observations and modeling of scintillation in the vicinity of a polar cap patch4
Nowcasting geoelectric fields in Ireland using magnetotelluric transfer functions4
Calibration of the GOES 6–16 high-energy proton detectors based on modelling of ground level enhancement energy spectra4
The Interplanetary and Magnetospheric causes of Geomagnetically Induced Currents (GICs) > 10 A in the Mäntsälä Finland Pipeline: 1999 through 2019 – Erratum4
Field-aligned scale length of depleted structures associated with post-sunset equatorial plasma bubbles4
Coordinated Ionospheric Reconstruction CubeSat Experiment (CIRCE), In situ and Remote Ionospheric Sensing (IRIS) suite4
New cosmic ray observations at Syowa Station in the Antarctic for space weather study4
Detecting undocumented trends in solar irradiance observations4
Climatology and modeling of ionospheric irregularities over Greenland based on empirical orthogonal function method4
HelioCast: heliospheric forecasting based on white-light observations of the solar corona3
Assessment of the radiation risk at flight altitudes for an extreme solar particle storm of 774 AD3
RMIT University’s practical space weather prediction laboratory3
First 3D hybrid-Vlasov global simulation of auroral proton precipitation and comparison with satellite observations3
Inferring depth-dependent plasma motions from surface observations using the DeepVel neural network3
An operational approach to forecast the Earth’s radiation belts dynamics3
The Mansurov effect: Statistical significance and the role of autocorrelation3
Application of Classical Kalman filtering technique in assimilation of multiple data types to NeQuick model3
Interplanetarymedium monitoring with LISA: Lessons from LISA Pathfinder3
Statistical models of the variability of plasma in the topside ionosphere: 2. Performance assessment3
Interhemispheric variability of the electron density and derived parameters by the Swarm satellites during different solar activity3
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