Journal of Space Weather and Space Climate

Papers
(The TQCC of Journal of Space Weather and Space Climate is 4. 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
Norway spruce forest management in the Czech Republic is linked to the solar cycle under conditions of climate change – from tree rings to salvage harvesting26
Ionospheric plasma structuring in relation to auroral particle precipitation23
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 drifts22
Nowcasting geoelectric fields in Ireland using magnetotelluric transfer functions20
Development of accelerated methods for calculating the pattern of current spreading over the surface of spacecraft19
Storm time neutral density assimilation in the thermosphere ionosphere with TIDA17
SODA – A tool to predict storm-induced orbit decays for low Earth-orbiting satellites14
A new model for plasmapause locations derived from IMAGE RPI and Van Allen Probes data13
Exploring possibilities for solar irradiance prediction from solar photosphere images using recurrent neural networks13
Persistent high-latitude ionospheric response to solar wind forcing12
Geostationary electron dynamics: ICARE_NG² observations and new analytical model of daily electron fluxes driven by solar wind conditions12
Karl von Lindener’s sunspot observations during 1800–1827: Another long-term dataset for the Dalton Minimum11
ARAMIS: a Martian radiative environment model built from GEANT4 simulations10
Upwelling coherent backscatter plumes observed with ionosondes in low-latitude region9
Investigating the drivers of long-term trends in the upper atmosphere over Rome across four decades9
Identification of ionospheric scintillation in the low-latitude African sector using a commercial CubeSat constellation9
The spheroid CME model in EUHFORIA8
Characterization of local time dependence of equatorial spread F responses to substorms in the American sector8
The Mansurov effect: Seasonal and solar wind sector structure dependence8
A rare observation from mid-latitude of a blue aurora7
Forecasting solar energetic proton integral fluxes with bi-directional long short-term memory neural networks7
The Mansurov effect: Statistical significance and the role of autocorrelation6
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 sector6
Quasi-stationary substructure within a sporadic E layer observed by the Low-Frequency Array (LOFAR)6
Multi-instrument observations of ionospheric super plasma bubbles in the European longitude sector during the 23–24 April 2023 severe geomagnetic storm6
The refractive and diffractive contributions to GPS signal scintillation at high latitudes during the geomagnetic storm on 7–8 September 20176
The radiation environment over the African continent at aviation altitudes: first results of the RPiRENA-based dosimeter5
Assessment of models for the prediction of the Travelling Ionospheric Disturbance activity index in mid-latitude Europe4
Observations and modeling of scintillation in the vicinity of a polar cap patch4
Growin: Modeling ionospheric instability growth rates4
Climatology and modeling of ionospheric irregularities over Greenland based on empirical orthogonal function method4
Solar radio bursts impact on the International GNSS Service Network during Solar Cycle 244
Thermosphere model assessment for geomagnetic storms from 2001 to 20234
The time profile of relativistic solar particle events as observed by neutron monitors4
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 sector4
TSI modeling: A comparison of ground-based Ca II K-line data with space-based UV images from the SDO/AIA instrument4
Calibration of the GOES 6–16 high-energy proton detectors based on modelling of ground level enhancement energy spectra4
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