Journal of Space Weather and Space Climate

Papers
(The median citation count of Journal of Space Weather and Space Climate 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 2022-01-01 to 2026-01-01.)
ArticleCitations
Norway spruce forest management in the Czech Republic is linked to the solar cycle under conditions of climate change – from tree rings to salvage harvesting37
Variability in footpoint mapping of bursty bulk flows using Tsyganenko models: impact on swarm conjunctions30
A height-dependent climatological model of the equatorial ionospheric zonal plasma drifts (EZDrifts): Description and application to an analysis of the longitudinal variations of the zonal drifts25
Nowcasting geoelectric fields in Ireland using magnetotelluric transfer functions25
Development of accelerated methods for calculating the pattern of current spreading over the surface of spacecraft24
Ionospheric plasma structuring in relation to auroral particle precipitation24
Sun-to-Mud Observations of the May and October storms of 2024: impacts on Ireland's Space Weather22
A new model for plasmapause locations derived from IMAGE RPI and Van Allen Probes data22
Storm time neutral density assimilation in the thermosphere ionosphere with TIDA18
Persistent high-latitude ionospheric response to solar wind forcing18
SODA – A tool to predict storm-induced orbit decays for low Earth-orbiting satellites18
Climatological models of non-polar geomagnetic daily variations using the DIFI methodology with Swarm and CHAMP satellite data16
Geostationary electron dynamics: ICARE_NG2 observations and new analytical model of daily electron fluxes driven by solar wind conditions16
Exploring possibilities for solar irradiance prediction from solar photosphere images using recurrent neural networks15
Identification of ionospheric scintillation in the low-latitude African sector using a commercial CubeSat constellation14
Investigating the drivers of long-term trends in the upper atmosphere over Rome across four decades13
ARAMIS: a Martian radiative environment model built from GEANT4 simulations12
Karl von Lindener’s sunspot observations during 1800–1827: Another long-term dataset for the Dalton Minimum12
Upwelling coherent backscatter plumes observed with ionosondes in low-latitude region11
An explainable Machine Learning model for Large-Scale Travelling Ionospheric Disturbances forecasting11
Long-term trends of ionospheric electron density related to global warming10
The spheroid CME model in EUHFORIA10
New formulation for the topside ionosphere and plasmasphere based on NeQuick10
The Mansurov effect: Seasonal and solar wind sector structure dependence9
Characterization of local time dependence of equatorial spread F responses to substorms in the American sector9
A rare observation from mid-latitude of a blue aurora9
The Mansurov effect: Statistical significance and the role of autocorrelation8
The nature of the mesoscale field-aligned currents in the auroral oval for positive IMF BZ: More frequent occurrence in the dawnside sector than in the duskside sector8
Forecasting solar energetic proton integral fluxes with bi-directional long short-term memory neural networks8
Quasi-stationary substructure within a sporadic E layer observed by the Low-Frequency Array (LOFAR)8
The refractive and diffractive contributions to GPS signal scintillation at high latitudes during the geomagnetic storm on 7–8 September 20178
The radiation environment over the African continent at aviation altitudes: first results of the RPiRENA-based dosimeter8
Assessment of models for the prediction of the Travelling Ionospheric Disturbance activity index in mid-latitude Europe7
Solar radio bursts impact on the International GNSS Service Network during Solar Cycle 247
Multi-instrument observations of ionospheric super plasma bubbles in the European longitude sector during the 23–24 April 2023 severe geomagnetic storm7
On the detection of a solar radio burst event that occurred on 28 August 2022 and its effect on GNSS signals as observed by ionospheric scintillation monitors distributed over the American sector7
The L-Band solar flux retrieval from the Soil Moisture and Ocean Salinity (SMOS) mission: Theoretical algorithm and its validation7
Observations and modeling of scintillation in the vicinity of a polar cap patch6
Supersubstorms during the May 2024 superstorm6
Thermosphere model assessment for geomagnetic storms from 2001 to 20235
Climatology and modeling of ionospheric irregularities over Greenland based on empirical orthogonal function method5
The time profile of relativistic solar particle events as observed by neutron monitors5
Ionospheric response to the January 2022 geomagnetic storm using LOFAR and GNSS5
Real-time precise point positioning performance in Hong Kong during May 2024 space weather events5
TSI modeling: A comparison of ground-based Ca II K-line data with space-based UV images from the SDO/AIA instrument5
Climatology of the spread F over Roquetes, Spain: Impact of the medium scale traveling ionospheric disturbances5
Growin: Modeling ionospheric instability growth rates5
Assimilation of the total electron content obtained from GNSS to a model of the ionosphere using a hierarchical Bayesian network5
A modeling study of ≥2 MeV electron fluxes in GEO at different prediction time scales based on LSTM and transformer networks4
Medium-scale traveling ionospheric disturbances created by primary gravity waves generated by a winter storm4
The Solar Activity Monitor Network – SAMNet4
Calibration of the GOES 6–16 high-energy proton detectors based on modelling of ground level enhancement energy spectra4
New Swarm products NeGIX and TEGIX for monitoring horizontal ionospheric gradients4
Statistical models of the variability of plasma in the topside ionosphere: 1. Development and optimisation4
Intermittency in the integrated power of ionospheric density fluctuations4
Three-dimensional metal ion flow in the polar ionosphere simulated by a new ionospheric model4
Local environmental effects on cosmic ray observations at Syowa Station in the Antarctic: PARMA-based snow cover correction for neutrons and machine learning approach for neutrons and muons4
Signatures of wedgelets over Fennoscandia during the St Patrick’s Day Storm 20154
Helio1D modeling of temporal variation of solar wind: Interfacing between MULTI-VP and 1D MHD for future operational forecasting at L13
Association of the 11-year solar cycle with correlation and teleconnection structures in tropospheric circulation3
The polarisation of auroral emissions: A tracer of the E region ionospheric currents3
Global solar photospheric and coronal magnetic field over activity cycles 21–253
Ionospheric scintillation modeling. I. Validity of the plane wave approximation for an electromagnetic wave illuminating the ionosphere3
Estimating COSMIC Ionospheric Radio Occultation foF2 Error Using the Three-cornered Hat Method3
Influence of the Moon phase on ionospheric total electron content observed by GNSS remote sensing3
Multi-scale image preprocessing and feature tracking for remote CME characterization3
Orientation of the stream interface in CIRs3
A statistical study of polar cap flow channels observed in both hemispheres using SuperDARN radars3
The state of mid-latitude thermosphere retrieved from ionosonde and Swarm satellite observations during geomagnetic storms in February 20223
A regional space weather hazard variation index utilising Swarm FAST data3
Student-led design, development and tests of an autonomous, low-cost platform for distributed space weather observations3
Unexpected space weather causing the reentry of 38 Starlink satellites in February 20223
The effects of estimating a photoionization parameter within a physics-based model using data assimilation3
Lensing from small-scale travelling ionospheric disturbances observed using LOFAR3
Probabilistic hazard assessment: Application to geomagnetic activity3
Ionic liquid coating for charge mitigation of solar modules in space: Electron microscopy on insulating nanosphere lithography patterned surfaces3
Field-aligned scale length of depleted structures associated with post-sunset equatorial plasma bubbles3
BaLNet: A probabilistic Bayesian neural network for solar wind speed forecasting3
Upgrades of the ESPERTA forecast tool for solar proton events2
Prediction of even and odd sunspot cycles2
High precision, high time-cadence measurements of the MgII index of solar activity by the GOES-R Extreme Ultraviolet Irradiance Sensor 2: EUVS-C initial flight performance2
The high-energy proton instrument (HEPI), a compact Cherenkov radiation space weather monitor2
On the role of source surface height and magnetograms in solar wind forecast accuracy2
A Bayesian approach to the drag-based modelling of ICMEs2
Transition from westward to eastward tilts of equatorial plasma bubbles observed by an all-sky airglow imager2
The role of particle precipitation on plasma structuring at different altitudes by in-situ measurements2
Modeling of ionospheric scintillation2
An indicator of local auroral electrojet peak intensity and latitude inferred from scalar magnetometer measurements made by the Swarm satellites2
The implications of ionospheric disturbances for precise GNSS positioning in Greenland2
Reconstruction of electron precipitation spectra at the top of the upper atmosphere using 427.8 nm auroral images2
Climatology of large scale Traveling Ionospheric Disturbances above Europe during the 2014-2023 period2
No signature of extreme solar energetic particle events in high-precision 14C data from the Alaskan tree for 1844–1876 CE2
The Great Aurora of 4 February 1872 observed by Angelo Secchi in Rome2
The effects of solar radio bursts on frequency bands utilised by the aviation industry in Sub-Saharan Africa2
Interhemispheric variability of the electron density and derived parameters by the Swarm satellites during different solar activity – Erratum2
A climatological model of the equatorial electrojet based on Swarm satellite magnetic intensity observations2
Comparison of the modelled geoelectric fields of the Carrington and Halloween storms2
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