OOIR: Observatory of International Research

Papers

(The TQCC of Journal of Space Weather and Space Climate is 8. 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 2020-04-01 to 2024-04-01.)

Article	Citations
What sustained multi-disciplinary research can achieve: The space weather modeling framework	37
Accuracy assessment of the quiet-time ionospheric F2 peak parameters as derived from COSMIC-2 multi-GNSS radio occultation measurements	32
The Interplanetary and Magnetospheric causes of Geomagnetically Induced Currents (GICs) > 10 A in the Mäntsälä Finland Pipeline: 1999 through 2019	29
Graphical evidence for the solar coronal structure during the Maunder minimum: comparative study of the total eclipse drawings in 1706 and 1715	26
Changes in the Total Solar Irradiance and climatic effects	25
The flare likelihood and region eruption forecasting (FLARECAST) project: flare forecasting in the big data & machine learning era	24
Thermosphere modeling capabilities assessment: geomagnetic storms	19
The Dalton Minimum and John Dalton’s Auroral Observations	19
Timelines as a tool for learning about space weather storms	19
Sensing the ionosphere with the Spire radio occultation constellation	18
The Solar Activity Monitor Network – SAMNet	17
Is the F_10.7cm – Sunspot Number relation linear and stable?	17
The operational and research DTM-2020 thermosphere models	16
Gas-surface interactions modelling influence on satellite aerodynamics and thermosphere mass density	15
Geolectric field measurement, modelling and validation during geomagnetic storms in the UK	15
Solar Energetic Particle Event occurrence prediction using Solar Flare Soft X-ray measurements and Machine Learning	15
Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect	15
Unseasonal super ionospheric plasma bubble and scintillations seeded by the 2022 Tonga Volcano Eruption related perturbations	14
The Polar Cap (PC) index combination, PCC: relations to solar wind properties and global magnetic disturbances	13
A note on the sunspot and prominence records made by Angelo Secchi during the period 1871–1875	13
ORFEES – a radio spectrograph for the study of solar radio bursts and space weather applications	13
Long term variations of galactic cosmic radiation on board the International Space Station, on the Moon and on the surface of Mars	13
Global equivalent slab thickness model of the Earth’s ionosphere	13
Unexpected space weather causing the reentry of 38 Starlink satellites in February 2022	13
Geomagnetically induced currents during the 07–08 September 2017 disturbed period: a global perspective	13

Multi-instrument detection in Europe of ionospheric disturbances caused by the 15 January 2022 eruption of the Hunga volcano	12
Evaluating the relationship between strong geomagnetic storms and electric grid failures in Poland using the geoelectric field as a GIC proxy	12
A new climatological electron density model for supporting space weather services	12
Plasmasphere and topside ionosphere reconstruction using METOP satellite data during geomagnetic storms	11
SunCET: The Sun Coronal Ejection Tracker Concept	11
Space Weather research in the Digital Age and across the full data lifecycle: Introduction to the Topical Issue	10
Long-term studies of photospheric magnetic fields on the Sun	10
Reconstruction of the Parker spiral with the Reverse In situ data and MHD APproach – RIMAP	9
Timing of the solar wind propagation delay between L1 and Earth based on machine learning	9
Analytical and empirical modelling of the origin and heliospheric propagation of coronal mass ejections, and space weather applications	9
MITO: a new directional muon telescope	8
An integrated data-driven solar wind – CME numerical framework for space weather forecasting	8
On a limitation of Zeeman polarimetry and imperfect instrumentation in representing solar magnetic fields with weaker polarization signal	8