Parallel Sessions

Session Conveners: Simon Thomas,  Stephanie Yardley,  Immanuel C. Jebaraj

Description: Coronal mass ejections (CMEs) are large explosions of plasma and magnetic field from the Sun. Once ejected, they propagate through the heliosphere becoming ‘Interplanetary CMEs (ICMEs)’. ICMEs are responsible for the most severe space weather hazards in the vicinity of Earth and can pose serious threats to our technologies on ground and in space. In addition to solar flares, shock waves from CMEs can produce solar energetic particles (SEPs), which are accelerated to very high energies at these sites and then transported through the solar wind. The fluxes of SEPs are considerably higher than the background galactic cosmic ray flux and are therefore considered radiation hazards to humans and technology in space or at high-altitude. A combination of CMEs and SEPs pose substantial amounts of threat if Earth-directed, affecting the power-grid, transport and pipelines through ground-induced currents, radar and global navigation systems, and radiation hazards to spacecraft and astronauts. Recently, efforts have been made to understand, model and forecast the transport of CMEs and SEPs through the heliosphere and the associated impacts when they arrive at Earth and other planets. These advances have been rapid since the launches of Solar Orbiter and Parker Solar Probe, two new spacecraft which provide data from close to the Sun. Together with older multi-vantage point missions such as STEREO and the L1 spacecraft, understanding CME evolution, and SEP acceleration and propagation in the inner-heliosphere has taken a new turn. This session will provide an opportunity to share and discuss recent advances in both observations and modelling of these space weather events and their impacts, and to initiate collaborations between researchers and industry.

Full List of Oral Presentations:

Session Chairs: Simon Thomas,  Stephanie Yardley,  Immanuel C. Jebaraj

852	Monday	13:30-13:45	Saint Exupéry	The Effects of Solar Energetic Particles on Technology and Human Health- from Interplanetary Space to Ground Level	DYER Clive et al.	Oral
631	Monday	13:45-14:00	Saint Exupéry	Development of a new ground level neutron monitor	APSINALL Michael et al.	Oral
1020	Monday	14:00-14:15	Saint Exupéry	Solar Energetic Particle Analysis Platform for the Inner Heliosphere (SERPENTINE): results from the first three years	VAINIO Rami et al.	Oral
590	Monday	14:15-14:30	Saint Exupéry	Solar Energetic Particles: observations and results from the High-Energy Particle Detector (HEPD-01) onboard the CSES-01 satellite	MARTUCCI Matteo et al.	Oral (Virtual)
779	Monday	14:30-14:45	Saint Exupéry	Solar energetic particles acceleration by coronal shock waves	JARRY Manon et al.	Oral
652	Monday	15:00-15:15	Saint Exupéry	What CME properties account for the occurrence of SEP events?	RODRIGUEZ GARCIA Laura et al.	Oral (Virtual)
693	Monday	15:15-15:30	Saint Exupéry	Multi-spacecraft Observations of Energetic Particle Events Inside of 1 au: Measurements by Solar Orbiter, ACE and STEREO	HO George et al.	Oral
770	Monday	15:30-15:45	Saint Exupéry	Advancing SEP Event Forecasting: Introducing the PARASOL Model	WIJSEN Nicolas et al.	Oral
648	Monday	15:45-16:00	Saint Exupéry	Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection	MOROSAN Diana et al.	Oral
724	Monday	16:00-16:15	Saint Exupéry	Advancing Space Weather Forecasting: A Novel Magnetohydrodynamical Approach for Predicting CME-driven Geomagnetic Storms	ROY Souvik et al.	Oral (Virtual)
772	Wednesday	14:00-14:15	Saint Exupéry	Investigating ICME complexity and connectivity evolution during propagation	WINSLOW Reka et al.	Oral
616	Wednesday	14:15-14:30	Saint Exupéry	Multi-point Investigation of CME Alfvénicity and Coherence near 1 au	SCOLINI Camilla et al.	Oral
625	Wednesday	14:30-14:45	Saint Exupéry	Expansion and shrinkage of the sheath and magnetic cloud due to the interaction of two interplanetary coronal mass ejections	KIM Roksoon et al.	Oral
830	Wednesday	14:45-15:00	Saint Exupéry	Flux rope modeling of the 2022 Sep 5 CME observed by PSP and Solar Orbiter from 0.07 to 0.69 AU	DAVIES Emma et al.	Oral
867	Wednesday	15:00-15:15	Saint Exupéry	High spatial – temporal resolution Coronal Mass Ejections observed by the Metis coronagraph on board Solar Orbiter	RUSSANO Giuliana et al.	Oral
747	Wednesday	15:15-15:30	Saint Exupéry	Physics-driven machine learning for the prediction of coronal mass ejections’ travel times	PIANA Michele et al.	Oral
633	Wednesday	15:30-15:45	Saint Exupéry	3DCOREapp: Reconstruct CMEs using the « 3D Coronal Rope Ejection Model »	RÜDISSER Hannah et al.	Oral

SWR-02 poster presentations will be displayed during Poster I (Monday, Tuesday, Wednesday):

Session Chairs: Simon Thomas,  Stephanie Yardley,  Immanuel C. Jebaraj

603	Poster I	Multi-catalog analysis of Interplanetary Coronal Mass Ejections: First statistical results	LARRODERA Carlos et al.	In Person
619	Poster I	Modeling the CME propagation in the heliosphere with COCONUT: Implementation of the RBSL flux rope model and event study	GUO Jinhan et al.	In Person
653	Poster I	Global simulation of the solar wind: A comparison with Parker Solar Probe observations	WU Chin-Chun	In Person
660	Poster I	Modelling two energetic storm particle events observed by Solar Orbiter	DING Zheyi et al.	In Person
673	Poster I	Magnetic connectivity and sources of extended 3He-rich time periods observed by Solar Orbiter	KOULOUMVAKOS Athanasios et al.	In Person
679	Poster I	Predicting the geomagnetic effects of solar coronal mass ejections	MOSTL Christian et al.	In Person
680	Poster I	Shock and SEP Modeling of the September 5, 2022 solar event	KOULOUMVAKOS Athanasios et al.	In Person
694	Poster I	A comprehensive study from the Sun to the Earth of the Space Weather event starting on the 6 September 2017	LAURENZA M. et al.	In Person
700	Poster I	Discrepancies in the Properties of the 2021 November 3–5 Coronal Mass Ejection on Scales of 0.03 au Revealed by Simultaneous Measurements at Solar Orbiter and Wind	REGNAULT Florian et al.	In Person
702	Poster I	Analysis of two interacting Coronal Mass Ejections through novel Extreme Ultraviolet Imager observations and modelling	DORSCH Brenda et al.	In Person
705	Poster I	Observations of Forbus decreases during 23rd and 24th solar cycles from PAMELA and AMS-02 space-borne detectors	MARTUCCI MATTEO et al.	In Person
714	Poster I	Predicting CME flux rope signatures using 3DCORE	AMERSTORFER Ute V. et al.	In Person
738	Poster I	MHD simulation of the Sun-to-Earth propagation of a CME through a data-driven reconstruction of the ambient solar wind	BIONDO Ruggero et al.	In Person
773	Poster I	Towards new insights into SEP events with the Icarus+PARADISE simulation model	HUSIDIC Edin et al.	In Person
775	Poster I	Extension of ESA’S Solar Accumulated And Peak Proton And Heavy Ion Radiation Environment (SAPPHIRE) model: The SAPPHIRE-2S model	AMINALRAGIA-GIAMINI et al.	In Person
778	Poster I	Understanding CME erosion and its impact on geo-effectiveness using EUHFORIA	MAHARANA Anwesha et al.	In Person
782	Poster I	Modeling flank encounters of CMEs with EUHFORIA	VALENTINO Angelo et al.	In Person
807	Poster I	Citizen science approach for Galactic Cosmic radiation and SEP monitoring at commercial flight altitude: the “Cosmic in the air” project	TROMPIER François et al.	In Person
842	Poster I	Modelling the 2011 September 6 SEP event with QVR-PARADISE	ARAN Angels et al.	In Person
855	Poster I	CHARACTERIZATION OF SOLAR EVENTS AND THEIR IMPACTS ON THE EARTH’S MAGNETIC FIELD USING DATA PROVIDE BY AMBER STATION IN YAOUNDE-CAMEROON	TCHANA Christian Brice et al.	In Person
893	Poster I	Study of 28 th September 2021 CME-driven shock: kinematics reconstruction and plasma parameters derivation by using multi-instruments observations	FRASSATI Federica et al.	In Person
916	Poster I	Effect of the heliospheric sector boundary on the propagation of solar energetic particles	LIOU Kan et al.	In Person
919	Poster I	Forecasting of solar wind velocity based on L5-L1 simulations	PODLADCHIKOVA Tatiana et al.	In Person
928	Poster I	Estimating the Near-Sun axial magnetic field of a CME observed on 10 March 2022 by invoking magnetic-helicity conservation.	KOYA Shifana et al.	In Person
930	Poster I	Understanding SEP propagation in CME-CME interaction scenarios.	NIEMELA Antonio et al.	In Person
934	Poster I	An Open-Source Python Wrapper for MAGNETOCOSMICS, for Calculating Cut-off Rigidities and Asymptotic Directions in Earth’s Magnetosphere	DAVIS Chris et al.	In Person
939	Poster I	Analysis of cosmic ray measurements on board aircraft using Citizen Science gas detectors: an overview of calibration issues	TROMPIER François et al.	In Person
968	Poster I	Multi-Spacecraft Observation of Three SEP Events and Associated CMEs in Late March 2022	LIGHT Christopher et al.	In Person
970	Poster I	Coronal dimmings as indicators of early CME propagation direction	PODLADCHIKOVA Tatiana et al.	In Person
997	Poster I	Anisotropies of cosmic ray flux: observations made from the space weather laboratory installed at the Argentine Marambio Antarctic base	SANTOS Noelia et al.	In Person
1013	Poster I	Radio emissions triggered by the solar events	LAZAR Marian et al.	In Person
1019	Poster I	CCMC Scoreboards	MAYS Leila et al.	In Person
1027	Poster I	Propagation of solar energetic particles in 3D MHD simulations of the solar wind.	HOUEIBIB Ahmed et al.	In Person
1092	Poster I	Exploring CME evolution from Sun to Earth using a very large simulation database	GIBSON Sarah et al.	In Person
1102	Poster I	Model comparison for geoeffective fast halo CMEs during solar cycle 24	YORDANOVA Emiliya et al.	In Person
1129	Poster I	Magnetic Properties of Source Regions of CMEs Associated with/without DH Type II Radio Bursts	VIJAYALAKSHMI P. et al.	In Person
1162	Poster I	CMEs and CIRs observed at the Earth, Venus and Mars for the PLATINUM project	RODRIGUEZ Luciano et al.	In Person
1175	Poster I	Parker Solar Probe Analysis of Magnetic Switchbacks in the Vicinity of Coronal Mass Ejections	MCDOUGALL Emily et al.	In Person
1254	Poster I	Solar Energetic (∼ 25 MeV) Proton Events Observed by the High Energy Telescopes on the STEREO Spacecraft or at the Earth During the First Solar Orbit of STEREO A (2006–2023)	RICHARDSON Ian et al.	In Person
1255	Poster I	Proton energy spectra of energetic storm particle events and their relation with magnetic field turbulent fluctuations nearby the associated interplanetary shocks	LEPRETI Fabio et al.	In Person
1259	Poster I	Bayesian approach to Propagation of Coronal Mass Ejections	CHIERICHINI Simone et al.	In Person
1275	Poster I	Open-Source Analysis Platform for Solar Energetic Particles provided by SERPENTINE	GIESELER Jan et al.	In Person
1294	Poster I	Automatic Multi-Instrument CME Feature Tracking and Velocity Estimation With Algorithmic and Deep Learning Approaches	STEPANYUK Oleg et al.	In Person
1296	Poster I	Solar observations at the ISS Solar Observatory in Magurele, Romania	TEODORESCU Maximilien et al.	In Person
NA	Poster I	Effects of adiabatic focusing and free-escape boundaries in coronal shock acceleration	ANNIE JOHN Lidiya et al.	In Person

Session Conveners: Eelco Doombos, Yaqi Jin, Lucilla Alfonsi

Description: The session focuses on the state-of-the-art understanding of the complex mechanisms ruling the Magnetosphere-Ionosphere-Thermosphere (M-I-T) coupling and how they translate into space weather impacts. Such an understanding is fundamental for the development of effective countermeasures against disruption, failure and deterioration of vulnerable technologies, such as GNSS critical applications, HF/VHF/UHF radio communications and LEO satellites operations. In order to forecast, warn, and mitigate adverse space weather effects, a better understanding of the M-I-T coupling plays a key role. It is essential to improve the prediction of: geomagnetic storm-time behaviour of the occurrence of spread-F, polar cap patches and scintillation phenomena that can degrade navigation and communication systems, thermospheric density variability affecting satellite drag and the enhancement of field-aligned currents, just to mention a few examples. Another crucial aspect of M-I-T coupling is the interhemispheric symmetric/asymmetric response to variable drivers that, if properly predicted, could support regional space weather modelling. Contributed papers may address (but are not limited to) recent developments in modelling and forecasting, monitoring methodologies, data analysis, measurement campaigns and international initiatives related to M-I-T coupling and associated threats on systems, at regional and global scale.

Full List of Oral Presentations:

Session Chairs: Eelco Doombos, Yaqi Jin, Lucilla Alfonsi

789	Tuesday	16:45-17:00	Saint Exupéry	Scintillation Climatology from a Software Defined Radio Receiver over Antarctica	IMAM Rayan et al.	Oral
783	Tuesday	17:00-17:15	Saint Exupéry	Forecasting and mitigation Ionospheric scintillation at low latitude: a case study	SPOGLI Luca et al.	Oral
743	Tuesday	17:15-17:30	Saint Exupéry	Autonomous Service for Prediction of Ionospheric Scintillations (ASPIS)	MACKOVJAK Simon et al.	Oral
915	Tuesday	17:30-17:45	Saint Exupéry	Impact of auroral particle precipitation on plasma structuring in the cusp region studied by the SS-520-3 sounding rocket	BUSCHMANN Lisa M. et al.	Oral
881	Tuesday	17:45-18:00	Saint Exupéry	Characterisation of the permanent solar wind impact on the high-latitude electron density	BORRIES Claudia et al.	Oral
746	Wednesday	14:00-14:15	Cassiopée	Investigation of sub-auroral polarization streams (SAPS) combined with magnetic field data	SCHILLINGS Audrey et al.	Oral
554	Wednesday	14:15-14:30	Cassiopée	STEVE Events with FUV Emissions	ZHANG Yongliang et al.	Oral
922	Wednesday	14:30-14:45	Cassiopée	Ionospheric HF Doppler indication of GNSS positioning errors	URBAR Jaroslav et al.	Oral
573	Wednesday	14:45-15:00	Cassiopée	A World of Complexity: The Ionosphere Observed with the International LOFAR Telescope	WOOD Alan et al.	Oral
1004	Wednesday	15:00-15:15	Cassiopée	COSMIC-2 Multi-Instrumental Observation of Storm-Induced Ionospheric Plasma Bubbles at Equatorial and Middle Latitudes	ZAKHARENKOVA Irina et al.	Oral
657	Wednesday	15:15-15:30	Cassiopée	Characterizing the ionization anomaly crests using the Far Ultraviolet imager onboard ICON	WAUTELET Gilles et al.	Oral
739	Wednesday	15:30-15:45	Cassiopée	Electrodynamic coupling from the high to middle latitudes: Observations in the Context of Whole Atmosphere Modelling	WALACH Maria-Theresia et al.	Oral
560	Thursday	16:45-17:00	Saint Exupéry	Improvements of multi-scale geomagnetic forcing specification from the ground-based integrated networks and the impacts on I-T modeling	DENG Yue et al.	Oral
802	Thursday	17:00-17:15	Saint Exupéry	Thermosphere-Ionosphere Observing System Simulation Experiments with multi-satellite constellations	KODIKARA Timothy et al.	Oral
963	Thursday	17:15-17:30	Saint Exupéry	Radiation pressure modelling for improving neutral thermosphere density and crosswind data products.	HLADCZUK Natalia et al.	Oral
865	Thursday	17:30-17:45	Saint Exupéry	Swarm: new « Fast-track » data processing chain	QAMILI Enkelejda et al.	Oral
664	Thursday	17:45-18:00	Saint Exupéry	The CSES missions and their contribution as Space Weather sentinels	SOTGIU Alessandro et al.	Oral

SWR-03 poster presentations will be displayed during Poster I (Monday, Tuesday, Wednesday):

Session Chairs: Eelco Doombos, Yaqi Jin, Lucilla Alfonsi

551	Poster I	Ionosphere-Thermosphere Coupling via Global-Scale Waves: New Insights from Two-Years of Concurrent In-Situ and Remotely-Sensed Satellite Observations	GASPERINI Federico et al.	In Person
572	Poster I	Space weather disturbances in non-stormy times: Occurrence of dB/dt spikes during three solar cycles	SCHILLINGS Audrey et al.	In Person
588	Poster I	Observation of 3-4 days oscillations in the southern Hemisphere crest of Equatorial Ionization Anomaly	LOMOTEY Solomon Otoo et al.	In Person
592	Poster I	Assessment of the ionospheric scintillation on L-band signals over Portugal	MOROZOVA Anna et al.	In Person
593	Poster I	Ionosphere over Eastern North Atlantic mid-latitudinal zone during geomagnetic storms	MOROZOVA Anna et al.	In Person
596	Poster I	Climatological Variation of VTEC over Nepal : A Comparative Study with Prediction Models.	GHIMIRE Basu Dev et al.	In Person
638	Poster I	Impact of Flux Transfer Events on the Ionosphere: A Numerical Study	PAUL ARGHYADEEP et al.	In Person
641	Poster I	Solving the Bolzmann kinetic transport equation for exploring the space environment at Earth and planets	BENNE Benjamin et al.	In Person
662	Poster I	The importance of the polar regions to understand the magnetosphere-atmosphere coupling: the AGATA initiative	ALFONSI Lucilla et al.	In Person
703	Poster I	DAY TO DAY AND SEASONAL VARIATIONS OF GROWTH RATE OF THE RAYLEIGH-TAYLOR INSTABILITY IN THE EQUATORIAL IONOSPHERE	VITAL Luiz Fillip et al.	In Person
730	Poster I	Performance evaluation of different models on the prediction of the LSTIDs activity at mid-latitude Europe during geomagnetic storm events	AMARAL FERREIRA Arthur et al.	In Person
750	Poster I	Analysis of an artificially generated magnetosphere using plasma thrusters	RABUñAL GAYO Andrés et al.	In Person
751	Poster I	Impact on Mid-Latitude Ionospheric TEC and Scintillation during 2023 Geomagnetic Storms over France region	PASUMARTHI Babu Sree Harsha et al.	In Person
763	Poster I	Ionospheric irregularities with LOFAR and GNSS data: the case of the January 2022 storm	GHIDONI Rebecca et al.	In Person
801	Poster I	MHD instability modelling of intense solar events in support of the CAESAR project	IVANOVSKI Stavro et al.	In Person
816	Poster I	Climatological Characteristics of Large Scale Travelling Ionospheric Disturbances Detected by HF-Interferometry Method	SEGARRA Anton et al.	In Person
838	Poster I	Auroral emission polarisation from 2008 to this day: a handfull of discoveries and open prospectives…	BOSSE Leo et al.	In Person
844	Poster I	Observing the Sky with a Single LOFAR Station: Impact of Ionosphere on Position Measurements and Ionospheric State Analysis	POZOGA Mariusz et al.	In Person
882	Poster I	Dynamics and Asymmetry of the Main Ionospheric Trough: Insights into Earth-based Factors and Anomalies	PRZEPIóRKA Dorota et al.	In Person
889	Poster I	Relations of ionospheric activity with GNSS low-cost receivers positioning errors	TRýB Jakub et al.	In Person
897	Poster I	Ionospheric response to solar eclipse during 2014 to 2023 at low-mid latitude Indian station, Delhi.	GUPTA Ankit et al.	In Person
937	Poster I	Exploring Geomagnetic Variations Caused by Plasma Pressure Distributions Using Satellite Data and Numerical Modeling	ESPINOZA ACOSTA José Miguel et al.	In Person
949	Poster I	Confinement of the ionospheric responses over African & Asian regions due to the intense geomagnetic storm of August 2018	KADER Sk Samin et al.	In Person
976	Poster I	A Deep learning Approach to Predict the Topside Vertical Total Electron Content Based on Swarm-A measurements	ABU ELEZZ Ola et al.	In Person
979	Poster I	New Neutral Mass Density Estimates in the Framework of the Project ESPRIT	STRASSER Andreas et al.	Virtual
998	Poster I	Validation of Data Ingestion Technique into the NeQuick 2 Model over America by Means of TEC, Ionosonde and Radio Occultation Data.	OSANYIN Taiwo et al.	Virtual
1024	Poster I	Ionospheric Anomaly in Low-latitude Region over Nepal using GPS TEC Measurements	CHAPAGAIN Narayan et al.	In Person
1099	Poster I	South African Space Weather Ionospheric Monitoring in Near-Real-Time	MATAMBA Tshimangadzo Merline et al.	In Person
1100	Poster I	3. Solar Flare Effects on the Ionosphere	TSHISAPHUNGO Mpho et al.	In Person
1112	Poster I	How does auroral electron precipitation near the open–closed field line boundary compare to that within the auroral oval during substorm onset?	GRANDIN Maxime et al.	In Person
1131	Poster I	Geomagnetic and ionospheric response to the most intense solar flares during 2022	BOLINO Maria de los Angeles et al.	In Person
1135	Poster I	Trans-national access to plasmaspheric, ionospheric and thermospheric research facilities through PITHIA-NRF	TJULIN Anders et al.	In Person
1143	Poster I	Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary	BERENYI Kitti Alexandra et al.	In Person
1148	Poster I	Studying the ionospheric absorption variation using European Digisonde data during intense solar flares in September 2017	BARTA Veronika et al.	In Person
1149	Poster I	Proposal of a Diagram for Investigating Ionospheric Layer Behavior	ÖKTEN Mehmet Baran et al.	In Person
1170	Poster I	Scaling of Earth’s magnetosheath turbulence in simultaneous CLUSTER-MMS observations	TEODORESCU Eliza et al.	In Person
1204	Poster I	Whether sudden stratospheric warming effects are seen in the mid-latitude thermosphere of the opposite hemisphere?	PERRONE Loredana et al.	In Person
1217	Poster I	Study of equatorial ionospheric scintillations from 2012 to 2016 from Koudougou GPS station.	PAHIMA Tinlé et al.	In Person
1221	Poster I	Simulation of the formation and structuration of a diamagnetic cavity	MENU Melissa et al.	In Person
1232	Poster I	Space Weather Effects On the Plasmasphere-Ionosphere-Thermosphere System over the Northern Hemisphere during the November 2021 Geomagnetic Storm	SABBAGH Dario et al.	In Person
1250	Poster I	T-FORS: TRAVELLING IONOSPHERIC DISTURBANCES FORECASTING SYSTEM	FABBRO Vincent et al.	In Person
1253	Poster I	First results of Swarm Fast-track data: implementation and quality assessment	KERVALISHVILI Guram et al.	In Person
1264	Poster I	INGV HF products available on the ESA Space Weather Service Network portal	SCOTTO Carlo et al.	In Person
1269	Poster I	Aurora Nowcast smartphone App	WILLER Anna et al.	In Person
1271	Poster I	MAG-SWE-DAN	WILLER Anna et al.	In Person
1272	Poster I	Ion-neutral interactions in the Lower Thermosphere – Ionosphere: The need for in-situ measurements at altitudes below 200 km to resolve outstanding questions	SARRIS Theodoros et al.	In Person
1283	Poster I	Reconnection lines and flux rope axes via local coordinates in 6D Vlasiator results	ALHO Markku et al.	In Person
1285	Poster I	Lifetime of Energetic Electrons Due to Their Interactions with Chorus Waves	WANG Dedong et al.	In Person
1288	Poster I	Study of the bimodal distribution of variability of ionospheric parameters at high latitudes measured by the Swarm satellites	KOTOVA Daria et al.	In Person
1292	Poster I	The analysis of the socioeconomic impacts of the upper atmosphere effects	MAINELLA Sara et al.	In Person
1300	Poster I	Evidence of auroral acceleration processes in the polar region during sub-Alfvénic solar wind flow	WATERS James et al.	In Person
	Poster I	Variable correlationship for collionless shock	PIPALIYA Jivraj et al.	In Person

Session Conveners: Rico Behlke, Geoff Crowley, Thomas Berger

Description: The number of spacecraft being launched into orbit is increasing exponentially. As a result, the possible impacts of hazardous space weather become more important, and an improved quality of space weather forecasting and nowcasting services is of higher importance, as highlighted, for example, by the loss of Starlink spacecraft in February 2022 during a relatively minor geomagnetic storm. Space weather effects can manifest themselves in many ways depending on the spacecraft orbit. Examples include challenges with respect to collision avoidance or even uncontrolled reentry due to increased atmospheric drag, communication and navigation disruptions (and resulting flight control problems) between ground stations or GNSS sources and spacecraft due to ionospheric irregularities, and incidents related to charged particles (surface and internal charging, single event and total dose events). This session invites presentations from spacecraft developers, operators, and users, describing requirements and best practices that anticipate and/or mitigate mission risk with respect to space weather effects (both pre-mission and real-time). We also invite presentations from researchers and commercial developers describing new space weather specification and forecasting capabilities and services enabled by novel observations, instruments, or models and data exploitation techniques.

Full List of Oral Presentations:

Session Chairs: Rico Behlke, Geoff Crowley, Thomas Berger

582	Tuesday	14:00-14:15	Cassiopée	THE IRENE-AE9/AP9 NEXT GENERATION RADIATION SPECIFICATION MODELS – PROGRESS REPORT	LEE Kerry et al.	Oral
654	Tuesday	14:15-14:30	Cassiopée	A New Diffusion Model for the Inner Electron Radiation Belt	GLAUERT Sarah et al.	Oral
685	Tuesday	14:30-14:45	Cassiopée	First updates from SODA – a forecast service to predict storm induced satellite orbit decays	KRAUSS Sandro et al.	Oral (Virtual)
836	Tuesday	14:45-15:00	Cassiopée	Space Weather Data offered by the Proba-V/EPT mission during almost a solar cycle: from flux time series to effects	BORISOV Stanislav et al.	Oral
917	Tuesday	15:15-15:30	Cassiopée	Internal charging dynamics impact on space-weather driven charging risk predictions, from PAGER to mission dedicated prediction services	TEZENAS DU MONTCEL Benoît et al.	Oral
940	Tuesday	15:30-15:45	Cassiopée	An Investigative Framework for Trapped Particle Radiation Modelling	PAPADIMITRIOU Constantinos et al.	Oral
941	Tuesday	15:45-16:00	Cassiopée	Estimating Electron Dose in Geostationary Orbit from GOES Fluxes	RODRIGUEZ Juan V. et al.	Oral
967	Tuesday	16:00-16:15	Cassiopée	Analysis of collision risk for LEO satellites due to atmospheric drag enhancement by space weather events	NWANKWO Victor et al.	Oral

SWR-04 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Rico Behlke, Geoff Crowley, Thomas Berger

574	Poster II	Modelling the variability of the topside ionosphere: Results from the Swarm-Variability of Ionospheric Plasma (Swarm-VIP) project	Wood Alan	In Person
600	Poster II	Ionospheric turbulent parameters as proxies for SBAS performances in equatorial regions	HECKER Louis et al.	In Person
632	Poster II	A Martian radiative environment model built from Geant4 simulations of cosmic-ray atmospheric shower	CHARPENTIER Gabin et al.	In Person
649	Poster II	Thermospheric mass density derived from tracking space debris	JOHLANDER Andreas et al.	In Person
669	Poster II	Mounting and casing system for custom GNSS receiver for UAV applications	KOBRLOVá Kateřina et al.	In Person
846	Poster II	Radiation belt modelling using global MHD and integrated particle simulations for the SWIMMR Sat-Risk project	DESAI Ravindra et al.	In Person
925	Poster II	Surface Charging Risk Prediction Service in PAGER and extension to advanced mission profils characterisations	TEZENAS DU MONTCEL Benoît et al.	In Person
964	Poster II	Consistent Communication in case of Extraordinary Space Weather Events	DE PATOUL Judith et al.	In Person
971	Poster II	Spacecraft Environment Telemetry Simulator	DOE Stewart et al.	In Person
977	Poster II	Evaluating Space Weather effects on the orbit of satellites	PAULO Simões et al.	In Person
1000	Poster II	New space weather forecasting and warning types and criteria that take into account social impacts	TSUGAWA Takuya et al.	In Person
1146	Poster II	Spacecraft Charging of the Morazán MRZ-SAT Satellite in Low Earth Orbit: Differential Charging as a function of Electron Anisotropy	DESAI Ravindra et al.	In Person
1279	Poster II	Reactivation of the group of “Ionospheric Scintillation Monitoring” (ISM) products for the ESA Space Weather portal	NAOURI ALI et al.	In Person
1286	Poster II	Contribution of DORIS System to Global Ionospheric Scintillation Mapping	CHERRIER MARIE et al.	In Person
1291	Poster II	Effects of solar and geomagnetic activity on aerodynamic collision avoidance manoeuvres	TURCO Fabrizio et al.	In Person
1293	Poster II	The SPace ENVironment Information System (SPENVIS) – a new framework.	DE DONDER Erwin et al.	In Person
1295	Poster II	PEMEM: Solar cycle phase dependent specification model of 1-100 keV electron flux	DUBYAGIN Stepan et al.	In Person
1299	Poster I req	The Human Interplanetary Exploration Radiation Risk Assessment System (HIERRAS) system	SIMON Clucas et al.	In Person

Session Conveners: Joana Alves Ribeiro, Roberta Tozzi, Fernando Pinheiro

Description: Geomagnetic storms have been known to impact grounded conductors since the 19th century. However, as our reliance on technological systems grows, the economic consequences of geomagnetic induced currents (GICs) can be severe, as demonstrated by the March 1989 magnetic storm. Several groups are computing GICs for their respective national power networks to mitigate these effects. However, limitations on the information provided by power transmission operators and ground conductivity models can lead to errors in estimations. Additionally, GICs can have an impact on other types of grounded infrastructure, such as pipelines and railways, inducing corrosion and stray current interference, respectively. This session seeks to address the impact of GICs on grounded infrastructure, examine sources of uncertainty in GIC computation, and discuss potential mitigation strategies.

Full List of Oral Presentations:

Session Chairs: Joana Alves Ribeiro, Roberta Tozzi, Fernando Pinheiro

659	Thursday	15:15-15:30	Guillaumet 1/2	Modelling pipe to soil potentials and GICs in New Zealand’s gas pipelines	DIVETT Tim et al.	Oral
617	Thursday	15:30-15:45	Guillaumet 1/2	The impacts of geomagnetically induced currents on UK railway track circuit signalling	PATTERSON Cameron et al.	Oral
851	Thursday	15:45-16:00	Guillaumet 1/2	Very Low Frequency Observations During an Active DC Injection Campaign that Simulated Geomagnetic Storm effects on High Voltage Transformers	CLILVERD Mark et al.	Oral
898	Thursday	16:45-17:00	Guillaumet 1/2	Observation of dB/dt localization and magnetospheric fast flow burst during a magnetotail reconnection event	CHIGOMEZYO Ngwira et al.	Oral (Virtual)
663	Thursday	17:00-17:15	Guillaumet 1/2	Characterising the distribution of extreme geoelectric field events in Sweden	LANABERE Vanina  et al.	Oral
920	Thursday	17:15-17:30	Guillaumet 1/2	Developing operational GIC monitoring and forecasting for ground-based technological infrastructure	RICHARDSON Gemma et al.	Oral
826	Thursday	17:30-17:45	Guillaumet 1/2	Multi-site transfer function approach for real-time modeling of the ground electric field induced by the laterally-nonuniform ionospheric source	MARSHALKO Elena et al.	Oral (Virtual)
795	Thursday	17:45-18:00	Guillaumet 1/2	Measured vs. Modeled Transformer Storm Responses in South Island, New Zealand	PRATSCHER Kristin et al.	Oral (Virtual)

SWR-05 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Joana Alves Ribeiro, Roberta Tozzi, Fernando Pinheiro

549	Poster II	GEOMAGNETICALLY-INDUCED EFFECTS RELATED TO DISTURBED GEOMAGNETIC FIELD VARIATIONS AT LOW LATITUDES	KOUASSI Nguessan et al.	In Person
608	Poster II	GIC mitigation in New Zealand: Working with Industry to develop new operational procedures	MAC MANUS Daniel et al.	In Person
615	Poster II	Sudden Commencements and Induced Currents: National Variability and Vulnerability in New Zealand	SMITH Andrew et al.	In Person
624	Poster II	Geomagnetically Induced Current research in New Zealand: the Solar Tsunamis research programme	RODGER Craig J. et al.	In Person
639	Poster II	Stream Interaction Region and Interplanetary Coronal Mass Ejections: two case studies	GHAMRY Essam et al.	Virtual
688	Poster II	Double H-spike disturbances at midlatitudes: their occurrence distribution, source, and space weather risk	GUERRERO Antonio et al.	In Person
735	Poster II	Delivering operational space weather products with the GorgonOps global magnetospheric simulation suite	LAMOURY Adrian et al.	In Person
757	Poster II	Frequency analysis of Geomagnetically Induced Currents in High Voltage Power lines in the UK	COLLINS Adam et al.	In Person
788	Poster II	Influence of Intense Geomagnetic Storms on Power Grid Malfunctioning in Poland during the Solar Cycle 24	GIL Agnieszka et al.	In Person
821	Poster II	An Overview of the Unique DC Injection Campaign for Replicating GICs on High Voltage Transformers in New Zealand	LAPTHORN Andrew et al.	Virtual
847	Poster II	Assessing hazards to ground-based infrastructure using the Magnetometer Network of Ireland	MALONE-LEIGH John et al.	In Person
868	Poster II	Network analysis of Geomagnetically induced currents in the US power grid	ORR Lauren et al.	In Person
900	Poster II	GIC estimation using differential magnetometer method under a 765 kV power line in South Africa	CILLIERS Pierre et al.	Virtual
1116	Poster II	3D MHD Modelling of the Earth’s magnetosphere: Ongoing Bergen-Imperial Global Geospace (BIGG) Project	KWAGALA Norah Kaggwa et al.	In Person
1119	Poster II	Phase gradient screen approach in modeling of ionospheric scintillation	VASYLYEV Dmytro et al.	In Person
1155	Poster II	Forecasting of ground level magnetic field perturbations caused by geomagnetic storms from L1 data using machine learning	FIELDING Samuel et al.	In Person
1181	Poster II	Influence of ground conductivity models on GIC hazard estimation in Germany	PICK Leonie et al.	In Person
1215	Poster II	Temporal changes in the tipper transfer function due to space weather: analysis using data from the Eskdalemuir magnetic observatory	WANG Guanren et al.	In Person
1223	Poster II	Does the vertical magnetic field component need to be considered in GIC studies?	CONNORS Martin et al.	In Person
1236	Poster II	Using Magnetotelluric Impedance Tensors for Surface Electric Field and GIC Prediction	WEIGEL Robert et al.	In Person
1239	Poster II	Modeling the geoelectric fields using the most recently acquired magnetotelluric data in the Iberian Peninsula	HAFIZI Raha et al.	In Person
1307	Poster II	Testing different metrics for 3D conductivity model comparison	ALVES RIBEIRO Joana et al.	In Person

Session Conveners: Guillerme Bernoux, Jorge Amaya, Christos Katsavrias

Description: Over the past decade, many studies have demonstrated that machine learning (ML), deep learning (DL), and more generally Artificial Intelligence (AI) have the potential to unlock new insights in space weather and space climate research. The goal of this session is to provide a platform for researchers and developers to present and discuss the latest breakthroughs in AI techniques for understanding, modelling, and predicting space weather and climate.

This session welcomes submissions on the use of ML/DL methods to model individual or multiple components of the Sun-Earth system. Problems to be addressed include: detection of solar structures, reconstruction of the solar and heliospheric topology, prediction of solar wind conditions at different locations, forecasting of energetic events multiple hours and days in advance, forecasting of the geomagnetic environment from information at L1 and from solar images, reconstruction of the current geomagnetic environment from ground and space-based observations, among others.

These models can be purely data-driven, but we also invite submissions that address the interaction of AI-based methods with traditional physical methods. This includes the use of ML/DL methods to accelerate and/or improve the accuracy of physical models, as well as the chaining of models of different nature and the quantification of uncertainty within complex pipelines. Submissions on methods that allow explicit inclusion of prior physical knowledge (such as so-called physics-informed or physics-aware methods) are strongly encouraged.

With ML/DL methods it also becomes possible to leverage vast amounts of data gathered over several solar cycles. Submissions on the creation and provision of large datasets, especially « ML-ready » ones, would be appreciated, as well as presentations on AI methods to refine and augment datasets (e.g. automatic calibration, cleaning, projection, etc.). Since it is difficult to label large datasets by hand, we also invite submissions on automating tasks such as detecting, segmenting and labelling solar regions or events of interest.

Last but not least, the community is already moving towards the implementation of ML/AI models into operation space weather services. In this perspective, validation of ML/AI results is critical. The results produced by these techniques must be validated against existing benchmarks and should be as explainable as possible. In short, they must demonstrate that they are trustworthy. We therefore support the submission of abstracts on the use of explainable AI for space weather and climate forecasting and, more generally, submissions on how to reliably and rigorously validate AI-based models.

Full List of Oral Presentations:

Session Chairs: Guillerme Bernoux, Jorge Amaya, Christos Katsavrias

567	Monday	13:30-13:45	Guillaumet 1/2	Space Weather modeling at the University of Colorado Deep Learning Laboratory	CAMPOREALE Enrico et al.	Oral
908	Monday	13:45-14:00	Guillaumet 1/2	Physics-informed neural networks for solar magnetic field simulations	JAROLIM Robert et al.	Oral
737	Monday	14:00-14:15	Guillaumet 1/2	Improving solar wind forecasting models with Neural Networks: towards physically accurate initial conditions and surrogate models.	S. BARROS Filipa et al.	Oral
858	Monday	14:15-14:30	Guillaumet 1/2	Investigation of the VAE and Their Potential for Space Weather Forecasting	EKATERINA Dineva et al.	Oral
621	Monday	14:30-14:45	Guillaumet 1/2	Reduced-Order Probabilistic Emulation of Physics-Based Ring Current Models	CRUZ Alfredo et al.	Oral
711	Monday	15:00-15:15	Guillaumet 1/2	Modelling Solar Images from SDO/AIA with Denoising Diffusion Probabilistic Models	RAMUNNO Francesco Pio et al.	Oral
626	Monday	15:15-15:30	Guillaumet 1/2	Neural network modeling of the ground magnetic perturbation at mid-latitude: towards future application of geomagnetic storm prediction	KIEOKAEW Rungployphan et al.	Oral
814	Monday	15:30-15:45	Guillaumet 1/2	Real-time high-resolution image reconstruction of ground-based solar observations for space weather applications	SCHIRNINGER Christoph et al.	Oral
955	Monday	15:45-16:00	Guillaumet 1/2	AI-generated Solar Farside Magnetograms by STEREO EUV Observations and Their Applications in the Corona and Heliosphere	JEONG Hyun-Jin et al.	Oral
727	Monday	16:00-16:15	Guillaumet 1/2	Physics-aware machine learning models for explainable solar flare forecasting	GUASTAVINO Sabrina et al.	Oral
740	Monday	17:00-17:15	Guillaumet 1/2	Recent advancements of a deep learning model to forecast the radiation belts electron fluxes at LEO with PROBA-V/EPT data	BOTEK Edith et al.	Oral (Virtual)
748	Monday	17:15-17:30	Guillaumet 1/2	CAMEL-II: A 3D CME catalog based on the CME automatic detection with a Transformer model	JIAHUI Shan et al.	Oral
969	Monday	17:30-17:45	Guillaumet 1/2	Advanced Multi-Instrument solar image segmentation and feature tracking for remote CME characterization: a hybrid CNN/algorithmic approach.	STEPANYUK Oleg et al.	Oral (Virtual)
888	Monday	17:45-18:00	Guillaumet 1/2	Knowledge discovery with additive attribution methods for geomagnetic index prediction	LOTZ Stefan et al.	Oral (Virtual)
728	Monday	18:00-18:15	Guillaumet 1/2	Facing imbalanced datasets in solar flare forecasting via score-oriented losses and value-weighted skill scores	MARCHETTI Francesco et al.	Oral

SWR-06 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Guillerme Bernoux, Jorge Amaya, Christos Katsavrias

565	Poster II	Derivation of Near Real-time ionospheric TEC from Single GNSS Receiver with Neural Network	MA Guanyi et al.	In Person
591	Poster II	Machine Learning applied for embedded radiation monitor particle species classification	MANSOOR Shahjahan et al.	In Person
614	Poster II	A machine-learning model for low-energy proton fluxes at low Earth orbit	BRUNET Antoine et al.	In Person
618	Poster II	Enhancing Observational Capabilities of EUV-observing Satellites to Estimate Spectral Irradiance	TREMBLAY Benoit et al.	In Person
622	Poster II	A Surrogate Model For Studying Solar Energetic Particle Acceleration and Transport	PODUVAL Bala et al.	In Person
635	Poster II	Classification methods as a surrogate of autorregression in uncertain solar wind speed forecasting	COBOS MAESTRE Mario et al.	In Person
642	Poster II	AIDefSpace: predicting the impact of space weather on telecommunications using machine learning	LAPENTA Giovann et al.	Virtual
651	Poster II	Using Convolutional Neural Networks for Image-Based Forecasting of Coronal Mass Ejections in Active Regions	HERNANDEZ CAMERO Julio et al.	In Person
661	Poster II	Solar features extraction for geomagnetic activity prediction: Using AutoEncoders to enhance data-driven models	TAHTOUH Maria et al.	In Person
704	Poster II	A transformer neural network for electron density prediction	JIN Mingwu et al.	In Person
708	Poster II	Enhancing STEREO-HI data with machine learning for efficient CME forecasting	LE LOUëDEC Justin et al.	In Person
719	Poster II	Automated Detection and Tracking of CMEs in HI	BAUER Maike et al.	In Person
728	Poster I req	Facing imbalanced datasets in solar flare forecasting via score-oriented losses and value-weighted skill scores	MARCHETTI Francesco et al.	In Person
745	Poster II	Forecasting Solar Proton Flux Time Profile through a Machine Learning Regression Algorithm	STUMPO Mirko et al.	In Person
791	Poster II	Short-term Forecasting of Solar Energetic Proton Integral Flux Using Deep Learning	NEDAL Mohamed et al.	In Person
848	Poster II	Neural networks for operational SYM-H forecasting	COLLADO-VILLAVERDE Armando et al.	In Person
880	Poster II	ARCAFF: Active Region Classification and Detection using Deep Learning	MALONEY Shane et al.	In Person
926	Poster II	Adapting object detection techniques to time series: application to the multi-class detection of ICMEs and CIRs	NGUYEN Gautier et al.	In Person
962	Poster II	Learning spatiotemporal null graphs of 3D magnetic skeletons extracted from high-fidelity plasma simulations	BOURI Ioanna et al.	Virtual
965	Poster II	Disturbance Storm Time index estimates from Cosmic Ray Data using Artificial Neural Networks	SABEHA Hadeer et al.	In Person
994	Poster II	AI on-board for near real-time CME detection	SANNER Martin et al.	In Person
1015	Poster II	SEP Prediction Using the New SHMARPs Dataset	KASAPIS Spiridon et al.	In Person
1018	Poster II	A Stacked Machine Learning Model for Vertical Tot	ASAMOAH Eric Nana et al.	In Person
1046	Poster II	A Deep Learning Model Based on Multi-Head Attention for F10.7 forecasting up to 27 days	MARCUCCI Adriana et al.	In Person
1114	Poster II	Development of Equatorial Spread F Prediction Model using Deep Learning at Chumphon Station, Thailand	THAMMAVONGSY Phimmasone et al.	In Person
1115	Poster II	Equatorial Plasma Bubble (EPB) for Classification by using Artificial Intelligence (AI)	THANAKULKETSARAT Thananphat et al.	In Person
1172	Poster II	Major solar flare forecast using deep reinforcement learning for imbalanced classfication	YI Kangwoo et al.	In Person
1207	Poster II	Sudden Storm Commencements detection with SVM classifiers using ground magnetic data.	TOURNIER Frédéric et al.	In Person
1210	Poster II	Operational radio solar flux at 30cm forecasting using Artificial Intelligence	SOUISSI Roiya et al.	In Person
1246	Poster II	Segmentation algorithm for various structures in solar atmosphere based on deep learning	BUTKA Peter et al.	In Person
1258	Poster II	Nowcasting and forecasting high energy electrons fluxes near magnetic equator with deep learning model using JASON/CARMEN and NPOES15/SEM2 data	MORIOUSEF Florian et al.	In Person
1273	Poster II	Information-theoretic measures for electron acceleration in the outer radiation belt	PAPADIMITRIOU Constantinos et al.	In Person

Session Conveners: Stephan G. Heinemann, Eleanna Asvestari

Description: The heliospheric solar wind structure, that is formed by the interaction of slow and fast wind, is the primary cause of minor to moderate geomagnetic activity and provides the medium in which other solar transients propagate. Stream interaction and co-rotating interaction regions produce shocks, compression, and rarefaction regions that are well known sources of recurrent geomagnetic effects on Earth. Therefore, understanding the heliospheric solar wind, ambient magnetic field, and their sources are vital in validating and refining space weather forecasting efforts. The aim of this session is to address the origin, evolution and space weather effects of fast and slow solar wind through the means of observations and models. Newly launched missions including Parker Solar Probe (PSP) and Solar Orbiter (SolO), as well as, established missions such as the Solar Dynamics Observatory (SDO) and the Solar Terrestrial Relations Observatories (STEREOs) provide a multitude of information that may be used to validate, improve, and refine current knowledge in this field. We encourage submissions regarding solar wind sources, both for slow and fast wind, solar wind acceleration/outflow, stream interaction, and the structure of the magnetic field and plasma topology at the source surface and the inner heliosphere. We welcome research that combines observations and models to further the understanding of solar and heliospheric physics in the framework of space weather.

Full List of Oral Presentations:

Session Chairs: Stephan G. Heinemann, Eleanna Asvestari

607	Monday	17:00-17:15	Saint Exupéry	Magnetic Reconnection and jetlets as the Driver of the Solar Wind	RAOUAFI Nour E. et al.	Oral
1007	Monday	17:15-17:30	Saint Exupéry	Statistical magnetic connectivity study from in-situ measurements of Solar Orbiter extrapolated sunward the Solar Corona.	DAKEYO Jean-Baptiste et al.	Oral
837	Monday	17:30-17:45	Saint Exupéry	Which solar coronal holes are geoeffective?	HOFMEISTER Stefan et al.	Oral
674	Monday	17:45-18:00	Saint Exupéry	Dependence of Stream Interaction Region Evolutions on the Coronal Hole Morphologies	MILOSIC Daniel et al.	Oral
991	Monday	18:00-18:15	Saint Exupéry	Solar wind observed by PSP at close to the Sun distances	MAGDALENIC Jasmina et al.	Oral
891	Tuesday	16:45-17:00	Cassiopée	Radial and transverse components of solar wind flows in the acceleration region across the solar activity cycle, connections with open field geometry	PINTO Rui et al.	Oral
681	Tuesday	17:00-17:15	Cassiopée	Impact of far-side active regions seen by Solar Orbiter on solar wind simulations	PERRI Barbara et al.	Oral
993	Tuesday	17:15-17:30	Cassiopée	Time-dependent solar wind simulations: improving forecasts and physical understanding of the solar wind in the heliosphere	SAMARA Evangelia et al.	Oral
586	Tuesday	17:30-17:45	Cassiopée	Investigating Helium Abundances in the Sun’s Atmosphere & Solar Wind Using the IRAP Solar Atmosphere Model & Solar Orbiter Data	THOMAS Simon et al.	Oral
575	Tuesday	17:45-18:00	Cassiopée	Understanding the Dynamics of Helium Abundance in Stream Interaction Regions: Insights	YOGESH et al.	Oral

100CD-02 poster presentations will be displayed during Poster I (Monday, Tuesday, Wednesday):

Session Chairs: Stephan G. Heinemann, Eleanna Asvestari

568	Poster I	Five-days ahead prediction of ambient solar wind with Physics-Informed Machine Learning	CAMPOREALE Enrico et al.	In Person
577	Poster I	Investigation of variations in Solar and Geomagnetic Parameters for Solar Cycle 24	SONDHIYA Deepak Kumar et al.	Virtual
630	Poster I	On the evolutionary aspects of solar coronal holes: A fast rotating and decaying coronal hole	HEINEMANN Stephan G. et al.	In Person
752	Poster I	Evidence of wave-wave modulation from observations of solar wind turbulence and waves during the September 2017 solar flares and CMEs	LOTOANIU Paul et al.	In Person
797	Poster I	On the Solar Open Magnetic Flux Problem	CHARLES Arge et al.	In Person
835	Poster I	Comparison of open and closed field topologies obtained with different coronal models	ASVESTARI Eleanna et al.	In Person
843	Poster I	Skewed Solar Wind proton populations: the Normal Inverse-Gaussian Model	LOUARN Philippe et al.	In Person
874	Poster I	Modelling the formation and evolution of solar wind microstreams: from coronal plumes to propagating Alfvénic velocity spikes	GANNOUNI Bahaeddine et al.	In Person
883	Poster I	Solar wind magnetic field measurements at the L5 Sun-Earth Lagrange point in the context of the Vigil space weather mission	EASTWOOD Jonathan et al.	In Person
913	Poster I	Modeling the source temperature of slow and fast solar winds using a 16 moments multi-species fluid model	LOMAZZI Paul et al.	In Person
953	Poster I	Solar wind modelling at near-Sun distances using the COCONUT coronal model and the EUHFORIA heliospheric model	VALLIAPPAN Senthamizh Pavai et al.	Virtual
981	Poster I	An Improved Power-Law Model for Electron Density in Solar Wind via Quasi-Thermal Noise Spectroscopy	KRUPAROVA Oksana et al.	In Person
985	Poster I	An Artificial Neural Networks Approach for predicting the Relationship between Equatorial Coronal Holes and High-Speed Streams	ABDULMAJED Rehab et al.	In Person
1031	Poster I	Fast and slow solar wind electron temperature estimations from the low corona to 1 au derived by the DYN model	KATSIYANNIS Thanassis et al.	In Person
1222	Poster I	What We Think We Know About CIRs/SIRs	DE KONING Curt et al.	In Person
1240	Poster I	Comparing Parker Solar Probe solar wind measurements with an empirical solar-wind model and WISPR remote sensing observations	BOTHMER Volker et al.	In Person
1244	Poster I	Magnetic reconnection in the solar wind and its impact on CMEs	FARGETTE Naïs et al.	In Person
1277	Poster I	Solar wind propagation throughout the 3D inner heliosphere	OPITZ Andrea et al.	In Person

Session Conveners: Martin Reiss, Barbara Perri, Evangelia Samara

Description: Assessing the current state-of-the-art in space weather modelling is pivotal for driving progress in space weather research and awareness. However, the rate at which we develop and improve our current modelling assets has greatly outpaced the rate at which we develop our validation infrastructure. This session seeks to reverse this trend by inviting contributions on (1) recent advances in validation and performance assessment of space weather models, (2) the development of new validation metrics and procedures, (3) the usage of multi-spacecraft observations from current space explorers for model validation, (4) the role of data science methods in model validation, and (5) community-coordinated validation efforts for model assessment. By tying the expertise on model validation in space weather research together, this session aims to identify opportunities for future advancements.

Full List of Oral Presentations:

Session Chairs: Martin Reiss, Barbara Perri, Evangelia Samara

1002	Thursday	14:00-14:15	Cassiopée	Space Weather capabilities assessment at different stages of the Research-to-Operations transition pipeline	KUZNETSOVA Masha et al.	Oral
768	Thursday	14:15-14:30	Cassiopée	The hard seed of COCONUT: how much do we really know about the « lower corona »?	BRCHNELOVA Michaela et al.	Oral
845	Thursday	14:30-14:45	Cassiopée	Using Solar Orbiter data in EUHFORIA to improve solar wind forecasts at 1AU	NEUMANN Vanessa et al.	Oral
758	Thursday	14:45-15:00	Cassiopée	Ensemble modeling of the solar wind and CMEs with a MHD model	SACHDEVA Nishtha et al.	Oral
957	Thursday	15:15-15:30	Cassiopée	SPHINX: An SEP Model Validation Infrastructure developed through Community Challenges and the SEP Scoreboards	WHITMAN Kathryn et al.	Oral
589	Thursday	15:30-15:45	Cassiopée	Performance assessment of the Swarm-Variability of Ionospheric Plasma (Swarm-VIP) models of the topside ionosphere	SPOGLI Luca et al.	Oral
894	Thursday	15:45-16:00	Cassiopée	Recent Model Validation Efforts Related to Near-Earth Space Radiation and Plasma Environment: Progress and Challenges	ZHENG Yihua et al.	Oral
989	Thursday	16:00-16:15	Cassiopée	Validation of Simulation Results in Response to the COSPAR ISWAT Challenge	WANG Dedong et al.	Oral
1028	Thursday	16:45-17:00	Cassiopée	Estimation of radiation exposure to cosmic radiation in the atmosphere of several planets of the Solar System by using DYASTIMA/DYASTIMA-R	MAKRANTONI Panagiota et al.	Oral
658	Thursday	17:00-17:15	Cassiopée	Validation of the UMASEP Solar Radiation Storm Model in the Space Weather Proving Ground	MORELAND Kimberly et al.	Oral
862	Thursday	17:15-17:30	Cassiopée	Validation of the Prediction of Adverse effects of Geomagnetic storms and Energetic Radiation (PAGER) framework	SHPRITS Yuri et al.	Oral
656	Thursday	17:30-17:45	Cassiopée	An open-source framework for high-fidelity physics-based space weather modeling on GPU systems: validation and benchmarks	VILA-PEREZ Jordi et al.	Oral

100CD-03 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Martin Reiss, Barbara Perri, Evangelia Samara

646	Poster II	Bottlenecks in space weather model validation: Where do we stand and how do we move forward?	REISS Martin et al.	In Person
666	Poster II	Solar Predict: a service for forecasting the 11 yr cycle	BRUN Allan sacha et al.	In Person
712	Poster II	Identification of multipoint ICMEs to understand their large-scale magnetic field structure using in situ and imaging observations	WEILER Eva et al.	In Person
722	Poster II	ESA’s Virtual Space Weather Modelling Centre: running web-based model chains	VERBEKE Christine et al.	In Person
731	Poster II	Observing the electron radiation belts of Earth from the near side of the Moon via their synchrotron radiation	MARC Gwendoline et al.	In Person
733	Poster II	On the importance of magnetospheric convection electric field modelling for Space Weather capabilities	KIRAZ Rabia et al.	In Person
760	Poster II	A novel full MHD forecasting model chain from Sun to Earth: COCONUT+ Icarus	TINATIN Baratashvili et al.	In Person
790	Poster II	Modelling the L-band amplitude scintillation index from Swarm face plate measurements	IMAM Rayan et al.	In Person
800	Poster II	Implementing a new flux-rope model into global MHD simulations to study the space weather impact of CMEs	SARKAR Ranadeep et al.	In Person
811	Poster II	Prediction accuracy of the outer Van Allen belt dynamics	DAGLIS Ioannis et al.	Virtual
820	Poster II	The RB-FAN framework providing Space Weather information for radiation belts induced risks for Space Operators: current status and future plans	FERLIN Antoine et al.	In Person
828	Poster II	Modelling of solar cycle intensity and duration	OGUNJO Samuel et al.	In Person
834	Poster II	HelioCast: heliospheric forecasting based on white-light observations of the solar corona	REVILLE Victor et al.	In Person
854	Poster II	SPHINX-Web as a Display for SEP Validation Results and Tool for Human Exploration Missions	QUINN Philip et al.	In Person
959	Poster II	Supporting Space Weather Modelling at the Community Coordinated Modeling Center (CCMC)	PETRENKO Maksym at al.	Virtual
1089	Poster II	Integrated Model for the Solar Energetic Particles and Alfven Wave Turbulence in the Inner Heliosphere	TENISHEV Valeriy et al.	In Person
1164	Poster II	PLAnetary plasma Turbulence and Intermittency – coupling with interplanetary transients from data analysis and NUmerical Modelling (PLATINUM), a new BRAIN-BE collaborative project	ECHIM Marius et al.	In Person
1227	Poster II	Monitoring Geospace cold plasma using PLASMA products	HEILIG Balázs et al.	In Person
1274	Poster II	How do physics-based modelled geomagnetic conditions compare with corresponding and existing space weather products within the ESA Space Weather service network?	KWAGALA Norah Kaggwa et al.	In Person
1278	Poster II	Moon to Mars Space Weather Analysis Office: SEP Model Validation Efforts	CHULAKI Anna et al.	In Person
1287	Poster II	Forecast of the Geomagnetic Index ap during CME events	STASINAKIS Argyris et al.	In Person

Session Conveners: Antoine Brunet, Constantinos Papadimitriou, Rungployphan Kieokaew

Description: Accurate forecasting and modelling of space weather events are crucial for mitigating their impacts on critical infrastructure, including communication systems, power grids, and navigation systems. However, these predictions are subject to uncertainty arising from both the data used to model the space weather system and the models themselves. Addressing these uncertainties is crucial to build a better understanding of the complex near-Earth space environment, provide more accurate forecasts, and identify shortcomings in the available data and models for space weather. The field of uncertainty quantification provides tools to characterise the sources of uncertainty and their impacts on a system. It involves a range of statistical and mathematical techniques, including probabilistic modelling, sensitivity analysis and reliability analysis. In our scientific community, these tools have been applied on physical modelling pipelines, empirical and data-driven models, as well as data assimilation models. This session focuses on uncertainty quantification in space weather modelling and data analysis. We invite contributions that address the challenges of quantifying and managing uncertainties in space weather and space climate, including: – Assessment and validation of uncertainty estimates in models and data – Estimations of spatial and temporal uncertainty correlations, as well as correlations between uncertainties in different physical processes – Uncertainty propagation in data assimilation and numerical simulation pipelines – Sensitivity analysis for space weather and space climate applications – Reliability analysis for space weather effects modelling Finally, contributions on how to leverage uncertainty estimates to build innovative space weather products and services would be very much appreciated.

Full List of Oral Presentations:

Session Chairs: Antoine Brunet, Constantinos Papadimitriou, Rungployphan Kieokaew

698	Wednesday	14:00-14:15	Guillaumet	Uncertainties in Coronal Hole Boundaries	MUGLACH Karin et al.	Oral
987	Wednesday	14:15-14:30	Guillaumet	Understanding our capabilities in observing and modelling Coronal Mass Ejections	VERBEKE Christine et al.	Oral
935	Wednesday	14:30-14:45	Guillaumet	Newcomb-Benford Law as a generic flag for changes in the derivation of long-term space weather time series	CHAPMAN Sandra et al.	Oral
623	Wednesday	15:15-15:30	Guillaumet	Multivariate Probabilistic Forecasting of Solar Indices and Proxies with Neural Network Ensembles	MEHTA Piyush Mukesh et al.	Oral
583	Wednesday	15:30-15:45	Guillaumet	Ionospheric reference and SBAS ionospheric integrity assessment	VERNISSE Yoann et al.	Oral
927	Wednesday	15:45-16:00	Guillaumet	Uncertainty Modeling of Acceleration-derived Thermosphere Observations	SIEMES Christian et al.	Oral

100CD-04 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Antoine Brunet, Constantinos Papadimitriou, Rungployphan Kieokaew

569	Poster II	ACCRUE: Accurate and Reliable Uncertainty Estimate	CAMPOREALE Enrico et al.	In Person
676	Poster II	Forecasting the electron ring current using data assimilation and ensemble modelling in the context of the PAGER project	HAAS Bernhard et al.	In Person
706	Poster II	On the relationship between the magnetic and electric component of the radial diffusion coefficients in the outer Van Allen belt	KATSAVRIAS Christos et al.	In Person
710	Poster II	Comparison of real-time and historical solar flare catalogs	CORTI Claudio et al.	In Person
741	Poster II	Space Weather Prediction using Heliospheric Images: A Data Assimilation Approach	AMERSTORFER Tanja et al.	In Person
818	Poster II	RB-FAN performances assessment campaign: assessing objectively forecast accuracy for Space Weather applications	MAGET Vincent et al.	In Person
914	Poster II	Comparing extreme event statistics in Dst, SYM-H and SMR geomagnetic indices.	BERGIN Aisling et al.	In Person
951	Poster II	Calibrating ionosonde-derived ionospheric heights with Incoherent Scatter Radar	SCOTT Christopher et al.	In Person
956	Poster II	Investigating the acceleration efficiency of VLF/ULF waves on different populations of outer radiation belt electrons, through multi-point observations and modeling	NASI Afroditi et al.	Virtual
1008	Poster II	Ensemble Modeling for Ring Current Environment using Perturbed Solar Wind Drivers	GODINEZ Humberto et al.	In Person
1091	Poster II	Validation of CME and SEP propagation models in the VSWMC	CHABANSKI Sophie et al.	In Person
1144	Poster II	Coronal Mass Ejection (CME) onset characterisation from multiple vantage points. What have we learned from the ESA-funded “Use of L5 Data in CME Propagation Models” activity?	GONZI Siegfried et al.	In Person
1301	Poster II	Uncertainties and performance metrics for modeling of inner Earth’s magnetosphere keV electron fluxes varying by several orders of magnitude	GANUSHKINA Natalia et al.	In Person

Session Conveners: Aurélie Marchaudon, Lasse Clausen, Beatriz Sanchez-Cano

Description: Multi-point measurements in space are more and more required in the study of the Sun-Earth relations and their applications in the framework of Space Weather, either to ensure a better discrimination of the spatial and temporal effects as it is the case for example of satellite swarms or joint satellite-rocket measurements or to ensure a better spatio-temporal coverage of a specific study region with in particular satellite constellations. At the two extremes of the spectrum, we find purely scientific missions such as ESA-Cluster, ESA-Swarm, NASA-Themis, NASA-MMS or the future NASA-HelioSwarm and NASA-GDC missions and commercial constellations for which some data used to ensure the attitude of the satellites have been diverted to scientific uses (determination of the Earth’s parallel currents from magnetometers on board the IRIDIUM constellation: AMPERE project). With the emergence of New Space, including the rise of nanosatellites, it becomes possible to consider new multi-point projects to improve the space-time coverage of the Sun-Earth system, in particular, but not only, for the near-Earth environment (radiation belts, ionosphere-thermosphere) and to allow a more global description and a better assimilation of the associated data in the forecasting models of these regions. In this session, we call for all contributions presenting original space projects using multi-point (satellites, cubesat, rockets, and why not balloons or a combination of these different devices), with possible applications for Space Weather.

Full List of Oral Presentations:

Session Chairs: Aurélie Marchaudon, Lasse Clausen, Beatriz Sanchez-Cano

764	Tuesday	14:00-14:15	Guillaumet 1/2	Localizing Techniques for Type III Radio Bursts	KRUPAR Vratislav et al.	Oral
982	Tuesday	14:15-14:30	Guillaumet 1/2	Can we intercalibrate satellite measurements by means of data assimilation?	CASTILLO Angelica Maria et al.	Oral
604	Tuesday	14:30-14:45	Guillaumet 1/2	The Firefly (4π) Mission: Enabling a Holistic View of the Sun and its Environment	RAOUAFI Nour  E. et al.	Oral
825	Tuesday	14:45-15:00	Guillaumet 1/2	A Multi-purpose Heliophysics L4 mission	HWANG Junga et al.	Oral
1005	Thursday	14:00-14:15	Saint Exupéry	Geosynchronous and Low Earth Orbit Radio Occultation Observations for the Space Weather Applications	CHERNIAK Iurii et al.	Oral
978	Thursday	14:15-14:30	Saint Exupéry	Multi-spacecraft mission concepts for ESA’s Space Weather Monitoring System	HEIL Melanie et al.	Oral
980	Thursday	14:30-14:45	Saint Exupéry	Multi-point measurements of space radiation environment from ESA Next Generation Radiation Monitor units	SANDBERG Ingmar et al.	Oral
701	Thursday	14:45-15:00	Saint Exupéry	Monitoring of Ionospheric Gradients At SWARM (MIGRAS)	HOQUE M Mainul et al.	Oral

100CD-05 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Aurélie Marchaudon, Lasse Clausen, Beatriz Sanchez-Cano

667	Poster II	Swarm-SWITCH: A new tool for monitoring the weather in the thermosphere-ionosphere using in-situ satellite observations and models	DOORNBOS Eelco et al.	In Person
675	Poster II	Study of Ionospheric Irregularities in ASEAN’s Magnetic Equator and Low Latitude Regions During 2022 and 2023	MYINT LIN MIN MIN et al.	In Person
687	Poster II	On the 3D multi-scale dynamics of the rippling phenomenon on the bow-shock surface	CAZZOLA Emanuele et al.	In Person
690	Poster II	Impact of Interplanetary Coronal Mass Ejections (ICME) on the geomagnetic tail	ALQEEQ Soboh et al.	In Person
695	Poster II	Tracking Long-Lived Active Regions with Multi-Viewpoint Observations	FINLEY Adam et al.	In Person
755	Poster II	A Statistical Study of Pc5 ULF Waves in Earth’s Magnetosphere Using Nearly 30 Years of GOES Magnetometer Data	LOTOANIU Paul T.M. et al.	In Person
777	Poster II	Developing a Regional:Swarm FAST Data Hazard Variation Index	ORR Lauren et al.	In Person
827	Poster II	Latest Results on the Development of a Deep Space Penetrating particle Analyzer	HULSMAN Johannes et al.	In Person
831	Poster II	Novel multi-point observation of the magnetosphere-ionosphere coupling and auroral acceleration regions during the terrestrial response to the 28th October 2021 coronal mass ejection	WATERS James et al.	In Person
896	Poster II	The 3D Energetic Electron Spectrometer on board PROBA-3 and the increase in its mission outcome from multi-point measurements	BENCK Sylvie et al.	In Person
952	Poster II	Study of the terrestrial ring current by the magnetic field observations of multi-spacecraft missions	TOMASIK Mate et al.	In Person
983	Poster II	New instrumental models for mutual impedance experiments and quasi-thermal noise spectroscopy in magnetized plasma	DAZZI Pietro et al.	In Person
1012	Poster II	LEO constellation for space weather now- and forecasting	PETROV Vasily et al.	In Person
1021	Poster II	Wave-particle interactions within the plasmasphere and their impact on the radiation belts	RIPOLL Jean-Francois et al.	In Person
1026	Poster II	Advancing Space Weather Capabilities with the Geospace Dynamics Constellation	GARCIA-SAGE Katherine et al.	Virtuel
1059	Poster II	Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere	LIU Jiajia et al.	In Person
1249	Poster II	NOAA Uses, Needs, and Plans for ESA Vigil Lagrange Point 5 Observations	WANG Nai-Yu et al.	In Person
1260	Poster II	Unveiling plasma energization and energy transport with multi-scale observations in the Earth’s Magnetospheric System: the Plasma Observatory mission and its relevance for Space Weather.	MARCUCCI Maria Federica et al.	In Person
1262	Poster II	The M-MATISSE mission: Mars Magnetosphere ATmosphere Ionosphere an	SANCHEZ-CANO Beatriz et al.	In Person
1280	Poster II	The French contribution for the NASA HelioSwarm mission	LE CONTEL Olivier et al.	In Person

Session Conveners: Alexander Mishev, Florian Mekhaldi, Natalie Krivova

Description: Space Weather studies and tools rely on modern observations of geomagnetic effects of solar activity. These observations might, however, not cover the entire possible range of such events. We know, for example, that extreme events, several orders of magnitude stronger than everything we have observed directly during the last 80 years, can occur on the Sun on centennial and millennial time scales. These include extreme solar flares and related particle storms, as well as the accompanying enormous geomagnetic disturbances. The consequences of such extreme events can be dramatic for the modern technological society, yet they cannot be quantified based upon the existing experience based on direct measurements. Also extended periods of extreme solar activity in general, such as grand minima and maxima, need to be better understood. Although extreme events are studied using indirect proxy data, such measurements are quite robust because of the enormous strength of the events. The session will focus on extreme solar activity periods (such as grand maxima and minima) and extreme solar events, as well as their application to modern Space Weather problems, viz. in the context of their parameters, physical origin and consequences. We welcome studies related to long-term changes in solar activity, the exceptionally strong events in the past, the most violent events of the recent solar cycles, as well as studies of superflares on Sun-like stars. Comparisons of recent models with experimental results are also very welcome. The aim of the session is to stimulate research and discussion allowing assessment of new observational and theoretical constraints for practical Space Weather studies.

Full List of Oral Presentations:

Session Chairs: Alexander Mishev, Florian Mekhaldi, Natalie Krivova

672	Wednesday	14:00-14:15	Spot	Flux of solar energetic particles on different timescales: Direct and indirect data	USOSKIN Ilya et al.	Oral
636	Wednesday	14:15-14:30	Spot	Investigation of the archival data for the GLE#5 on 23 February 1956	HAYAKAWA Hisashi et al.	Oral
601	Wednesday	14:30-14:45	Spot	Investigating the Effect of GLEs on Radiation Doses at Aviation Altitudes Using Neutron Monitor Data Over Several Solar Cycles	LARSEN Nicholas et al.	Oral

100CD-06 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Alexander Mishev, Florian Mekhaldi, Natalie Krivova

548	Poster II	About the necessity to study space weather effects during major historical GLEs	MISHEV Alexander et al.	In Person
602	Poster II	Charting extreme space weather events- combining estimates of risk and narratives of impact over multiple solar cycles	CHAPMAN Sandra et al.	In Person
780	Poster II	Centennial Total Solar Irradiance variation: a paradigm shift in sun-climate research.	DEWITTE Steven et al.	In Person
947	Poster II	Ice core 36Cl concentrations set upper limit for Carrington Event’s fluence spectrum	MEKHALDI Florian et al.	In Person
1108	Poster II	Preparing a new solar forcing dataset running from 1850 – 2300	DUDOK DE WIT Thierry et al.	In Person
1165	Poster II	Updated Predictions for Solar Cycle 25 from NOAA’s Space Weather Prediction Center	MIESCH Mark et al.	In Person
1184	Poster II	Digitizing the Carrington 1859 storm: magnetogram records from Greenwich and Kew observatories	LAWRENCE Ewelina et al.	In Person
1213	Poster II	Alfvénic and compressive waves in corotating Solar Wind high-speed streams and their signature on low-frequency geomagnetic activity at high latitudes	CARNEVALE Giuseppina et al.	In Person
1226	Poster II	Radial Variations of the Heliospheric Current Sheet Tilt Angle During Solar Minimum Years: Magnetohydrodynamic Simulations	WU Chin-Chun et al.	In Person
1304	Poster II	The world-wide network of neutron monitors – services, events and data provision	SAPUNDJIEV et al.	In Person

Session Conveners: Marco Molinaro, Veronique Delouille, Baptiste Cecconi

Description: The wealth of Space Weather data has grown exponentially in the last two decades, both in terms of volumes and diversity. Data are heterogeneous under many aspects, including: acquisition (instrument observation), exploitation (for various scientific research fields or for operational aspects), and format. Data are made e-accessible through portals. Metadata (often produced from automated feature recognition code) as well as data analysis and simulation codes are made available from various repositories. The heterogeneity and increased volume in data requires however to think about how to better homogenise the various aspects of the data infrastructures, in order to provide the users with solutions that follow FAIR principles and leverage on open standards development. In this effort, connection to global communities and organisations (IHDEA, COSPAR-ISWAT, IPDA, IVOA-SSIG) and scientific-to-operational infrastructure bridging (ESA SSA-SWE) are keys in showing the current status of these activities and helping to identify common ways forward. This session proposes to bring together expertise in Space Weather, solar, heliospheric and planetary science data management and data exploitation and make an inventory of elements of space weather data infrastructure. We welcome contributions describing ongoing and foreseen activities in producing high level metadata via automated feature recognition catalogues, and in homogenising and standardising Space Weather resource discovery, access and use towards a FAIR interoperable approach.

Full List of Oral Presentations:

Session Chairs: Marco Molinaro, Veronique Delouille, Baptiste Cecconi

1003	Tuesday	15:15-15:30	Guillaumet	The Quality of Data Bases and the Accuracy of Predictions	MARTENS Petrus et al.	Oral (Virtual)
899	Tuesday	15:30-15:45	Guillaumet	Geo-Magnetic Effectiveness and CME propagation forecast: tools for space weather monitoring within the SWESNET Project	PINNA Federico et al.	Oral
677	Tuesday	15:45-16:00	Guillaumet	BiScEF – A new format for archiving and sharing scintillation data	JACOBSEN Knut Stanley et al.	Oral
725	Tuesday	16:00-16:15	Guillaumet	Towards building a comprehensive data model and infrastructure for collecting and querying event chains	MANEVA Yana et al.	Oral
670	Thursday	15:15-15:30	Saint Exupéry	ProSpecT: Simplifying Product Description and Metadata Generation for the CAESAR Project	FORMATO Valerio et al.	Oral
878	Thursday	15:30-15:45	Saint Exupéry	Strategies of Data Discovery, Accessibility and Use for the TSRS Coronal Radio Surveillance system	JERSE Giovanna et al.	Oral
873	Thursday	15:45-16:00	Saint Exupéry	FAIR approach for Low Frequency Radio Astronomy	CECCONI Baptiste et al.	Oral
853	Thursday	16:00-16:15	Saint Exupéry	The SOLARNET Virtual Observatory (SVO)	VANSINTJAN Robbe et al.	Oral

100CD-07 poster presentations will be displayed during Poster II (Thursday, Friday):

Session Chairs: Marco Molinaro, Veronique Delouille, Baptiste Cecconi

637	Poster II	FAIR support at the Heliophysics Digital Resource Library	IRELAND Jack et al.	In Person
665	Poster II	Creating a Database for the ASPIS Prototype: Unraveling the Sun-Earth Chain of Phenomena in Space Weather Study	DEL MORO Dario et al.	In Person
689	Poster II	BibHelioTech: cataloguing and documenting all heliospheric events ?	GéNOT Vincent et al.	In Person
697	Poster II	NOAA NCEI Heliophysics and Space Weather Satellite Data: Status, Recent Improvements and Upcoming Events	RODRIGUEZ Juan et al.	In Person
841	Poster II	The eSWua ionospheric observing infrastructure: updates and future perspectives	PICA Emanuele et al.	In Person
871	Poster II	SolarMonitor2	MALONEY Shane et al.	In Person
875	Poster II	VESPA as a Heliophysics resource registry	CECCONI Baptiste et al.	In Person
923	Poster II	Metis ground support to operations: the Metis Operations Facility (MOF)	PINNA Federico et al.	In Person
954	Poster II	SPACE WEATHER ACTIVITIES: AN OVERVIEW OF AFRICAN STATUS AND CASE STUDY OF NIGERIA	RABIU Babatunde et al.	In Person
988	Poster II	Reproducibility and requirements for a fair comparative evaluation of automated feature recognition codes: a machine learning viewpoint	PAIEMENT Adeline et al.	In Person
996	Poster II	Agile Collaboration: Citizen Science as a Transdisciplinary Approach to Heliophysics	LEDVINA Vincent et al.	In Person
1009	Poster II	Open solar data, data products, and tools at MEDOC	BUCHLIN Eric et al.	In Person
1085	Poster II	Space Weather research and resulting ESA Services – an R2O success story	TEMMER Manuela et al.	Virtual
1133	Poster II	The PITHIA e-Science Centre	KISS Tamas et al.	Virtual
1136	Poster II	Comprehensive Space Weather Monitoring and Analysis in Brazil and Neighboring Regions	COSTA Joaquim et al.	In Person
1198	Poster II	TSRS Heritage Archive service design	BERTOCCO Sara et al.	In Person
1230	Poster II	Towards Machine-Interpretable Coordinate Transform Metadata in Heliophysics	WEIGEL Robert et al.	In Person
1237	Poster II	HAPI – A Standard Time Series Data Access API for Heliophysics and Planetary Data	WEIGEL Robert et al.	In Person
1302	Poster II	Space weather data and the WMO Information System, metadata and data policy.	ANDRIES Jesse et al.	In Person
1309	Poster II	NOAA space weather next data management and data flow architecture	AZEEM Irfan et al.	In Person

Session Conveners: K.D. Leka, Kathryn Whitman, Sophie Murray

Description: Flare forecasting research has been invoking big data (in some cases covering multiple solar cycles), multiple wavelength and physical regimes (beyond white-light imaging and photospheric magnetic field maps), and many new machine learning approaches.  Have we achieved serious breakthroughs?  Are new methods, including machine learning, improving the forecast performance?  How do we know?  Where are the gaps?  What is needed to move forward: Tools, Data, Methodologies?  This session will consist of a single « state of the science » review talk and an invitation for anyone in the community to present 2-4 slide « lightning talks » addressing the « Breakthroughs » and « Identifying the Gaps » questions, with associated time for discussion.  More detailed presentations of new methods and research will be available by way of associated posters.

Full List of Oral Presentations:

Session Chairs: K.D. Leka, Kathryn Whitman, Sophie Murray

645	Wednesday	15:00-15:15	Spot	Solar Flare Prediction: Attempting a Current Snapshot of the State of the Science	GEORGOULIS Manolis K. et al.	Oral
754	Wednesday	15:15-15:30	Spot	Predicting large solar flares with cellular automatons and data assimilation	STRUGAREK Antoine et al.	Oral
765	Wednesday	15:30-15:45	Spot	Addressing Known Gaps in Flare Forecasting	LEKA KD et al.	Oral

100CD-08 poster presentations will be displayed during Poster I (Monday, Tuesday, Wednesday):

Session Chairs: K.D. Leka, Kathryn Whitman, Sophie Murray

766	Poster I	Snap, Crackle, Pop! Flare-Imminent vs. Flare-Quiet Conditions in the Upper Solar Atmosphere.	LEKA KD et al.	In Person
1086	Poster I	Investigating the level of applicability and importance of different 3D extrapolation models in term of flare prediction	KORSOS Marianna et al.	In Person
1147	Poster I	Flare Forecasts at Solar Patrol Service	PAVELKOVA Martina et al.	Virtual
1303	Poster I	The evolution of low-corona pre-flare signatures	KRISTA Larisza et al.	In Person
1267	Poster I	New approaches to Solar Flare Forecast	FRANCISCO Grégoire	In Person

Session Conveners: Tamal Basak, Carine Briand, Nina Aleksandra

Description:  The session focuses on the recent developments in the theoretical understanding and instrumentation regarding ground-based ionospheric monitoring to the investigation of the middle and lower ionosphere. The theoretical understanding encompasses advanced numerical modelling during ionospheric perturbations. It includes the ionospheric perturbations due to solar flares, gamma ray events, solar eclipse, seismic activities etc. Chemical dynamics of the lower ionosphere and its consequences are also included. The instrumentation theme covers the aspects starting from the hardware related development to computational facilities in comprehensive ionospheric monitoring through networking /campaigns and best practices in data handling. A specific discussion on Very Low Frequency (VLF) /Low Frequency (LF) instruments and networks is expected. The data analysis consists of the analysis of the ionospheric data monitored through ground based stations, namely, LF / VLF signal, GPS based Total Electron Content (TEC), ionic constituents etc. Application of the machine learning for simulating the perturbed ionospheric conditions is also included in this section.

Full List of Oral Presentations:

Session Chairs: Tamal Basak, Carine Briand, Nina Aleksandra

587	Monday	13:30-13:45	Cassiopée	Remote Sensing and Space Weather: Simultaneous Observations of VLF Emissions and Inner Radiation Belt Electron Flux Variations by the CSES-01 Satellite	BURGER William Jerome	Oral
808	Monday	13:45-14:00	Cassiopée	Impact of ionospheric irregularities on S band signals around the northern crest of Equatorial Ionization Anomaly	BISWAS Trisani	Oral
958	Monday	14:00-14:15	Cassiopée	Investigation of Plasma Bubbles over Egypt and Development of an Artificial Neural Network Approach for the Detecting of Plasma Bubbles	M. SALAH Hager et al.	Oral
806	Monday	14:15-14:30	Cassiopée	Observation and modeling of D-region ionospheric disturbances due to solar eclipses using VLF/LF network	PAL Sujay et al.	Oral
721	Monday	14:30-14:45	Cassiopée	Propagation effects of Very Low Frequency signal: an efficient tool for studying solar-lower ionosphere interaction	BASAK Tamal et al.	Oral Virtual

100CD-09 poster presentations will be displayed during Poster I (Monday, Tuesday, Wednesday):

Session Chairs: Tamal Basak, Carine Briand, Nina Aleksandra

564	Poster I	LiDAR sensors for space	PESANTEZ-CABRERA Pamela Carolina et al.	In Person
686	Poster I	Study of the General Behaviour of D-region Response Time Delay During Solar Flares	CHAKRABORTY Sayak et al.	Virtual
718	Poster I	Effect of ground conductivity on VLF propagation modelling	TEYSSEYRE Pauline et al.	In Person
819	Poster I	Effects of solar flares on the D-region ionosphere as measured by VLF remote sensing method	HALDAR Prabir Kumar et al.	In Person
903	Poster I	Comparative Analysis of 1D Var Ionospheric Electron Density Retrieval Method using GNSS RO data for Periods of Varying Solar Activity	GULATI Ishita et al.	In Person
943	Poster I	Traveling ionospheric disturbances in the far field induced by tsunamis	CASTILLO RIVERA Carlos et al.	In Person
1016	Poster I	Proposed development of a COntinuous Network of GNSS receivers over North Africa (CONGA)	JONAH Olusegun et al.	In Person
1017	Poster I	Initial results for a possible sub-ionospheric VLF receiving site at Sikkim University, Gangtok, India as obtained from standard simulation techniques	MUKHERJEE Rupak et al.	In Person
1228	Poster I	Design and development of the Ionospheric Recording Stations within the H037-MoNEWIC/eMONITOR project	TAGARGOUSTE Youssef et al.	In Person
1234	Poster I	CYprus Radar for Ionospheric Space Situational Awareness (CYRISSA)	HARALAMBOUS Haris et al.	In Person
1235	Poster I	NOAA’s SWFO Program Launching in 2024: Science Objectives and Data Products	VASSILIADIS Dimitris et al.	Virtual
1251	Poster I	GNSS-derived inferences about the ionosphere: dTEC statistics and what they can tell us.	KINSLER Paul et al.	In Person