===========================================================================
TABLE OF CONTENTS
1. Call for Abstracts: EGU26 - Session ST1.7: Collisionless shocks and associated transient phenomena at Earth and beyond, the Deadline for abstract submission is next week, 15 January 2026, at 13:00 CET.
2. Call for Abstracts: EGU26 - ST4.4 Are We Ready for the Next Extreme Space Weather Events? Current state-of-the-art forecasting frameworks, knowledge gaps, and plans for mitigation of future severe risks, the deadline is on Thursday, 15 January 2026, 13:00 CET.
3. Call for Abstracts: Advertisement for two sessions at EGU 2026, abstract deadline: 15 January 2026, 13:00 CET.
4. Call for Abstracts: EGU 2026 session ST4.6 Modelling and observations of the near-Earth space weather environment, deadline: January 15, 2026, 13:00 CET.
5. Call for Abstracts: Invitation to submit to EGU 2026 Session ST1.6: Observing and modelling coronal mass ejections from the Sun to the heliosphere, abstract submission deadline is Thursday, 15 January 2026, 13:00 CET.
6. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.7 –Global magnetospheric-ionospheric dynamics in simulations and observations, the deadline for the abstract submissions is 15 January 2026, 13:00 CET.
7. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.3 -- Magnetic reconnection and associated multi-scale coupling in the collisionless environments, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
8. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.9 – Inner magnetosphere, Ionosphere, and Atmosphere Coupling, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
9. Call for Abstracts: Invitation to submit to EGU 2026 Session ST3.3 – Modeling the Interconnected Thermosphere, Ionosphere, Plasmasphere and Magnetosphere, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
10. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.4 – Wave-particle interactions, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
11. SHIELD Webinar Invitation: SHIELD Webinar Featuring Alan Stern, on Friday, February 13th at Noon ET.
12. Call for Abstracts: COSPAR PSW.6 (2026), deadline: February 13.
13. Invitation: The SCOSTEP's 16th Quadrennial Solar-Terrestrial Physics Symposium, deadline of abstract submission: 26 January 2026 (extended from 10 January 2026).
14. Call for Proposals: Dissemination request - ISSI International Team Call for Proposals (2026), Proposal deadline is 13 March 2026.
15. Call for abstracts: 46th COSPAR Scientific Assembly, the abstract deadline is 13 February 2026.
16. Webinar: Solar Orbiter community building webinar #1 (2026), take place on Wednesday 4 February 2026 (14:00 - 14:30 CET).
===========================================================================
!!!Attention!!!
Submissions to the newsletter is only accepted via our official webpage.
Link to website: https://spaceweather.gfz.de/contact/submission-to-helio-europe-mailing-list
1. Call for Abstracts: EGU26 - Session ST1.7: Collisionless shocks and associated transient phenomena at Earth and beyond, the Deadline for abstract submission is next week, 15 January 2026, at 13:00 CET.
From: Ahmad Lalti, Northumbria University, <ahmad.lalti at northumbria.ac.uk>
Subject: EGU26 call for abstracts: Session ST1.7: Collisionless shocks and associated transient phenomena at Earth and beyond.
Abstract submission is now open for the EGU 2026 conference, to be held in Vienna, Austria, from 3 to 8 May 2026, both in person and online. We would like to invite you to submit an abstract to our session: ST1.7: “Collisionless shocks and associated transient phenomena at Earth and beyond”. If you want to read more about the session, you can follow this link: https://meetingorganizer.copernicus.org/EGU26/session/57168
To submit an abstract, you can follow this link:
https://meetingorganizer.copernicus.org/EGU26/abstractsubmission/57168
The Deadline for abstract submission is next week, 15 January 2026, at 13:00 CET.
Session conveners: Ahmad Lalti, Florian Koller, Artem Bohdan, Jonas Suni, Laura Vuorinen
2. Call for Abstracts: EGU26 - ST4.4 Are We Ready for the Next Extreme Space Weather Events? Current state-of-the-art forecasting frameworks, knowledge gaps, and plans for mitigation of future severe risks, the deadline is on Thursday, 15 January 2026, 13:00 CET.
From: Rungployphan Kieokaew, Research Institute in Astrophysics and Planetology (IRAP), France, <rkieokaew at irap.omp.eu>
Subject: EGU26 - ST4.4 Are We Ready for the Next Extreme Space Weather Events? Current state-of-the-art forecasting frameworks, knowledge gaps, and plans for mitigation of future severe risks.
We solicit abstracts for our EGU26 session on extreme space weather events and our preparedness for space weather forecasting tools and risk mitigation plans. The deadline is on Thursday, 15 January 2026, 13:00 CET.
Short description of our session:
Extreme space weather events, such as X-class flares and Kp9 geomagnetic storms, pose systemic risks to global power grids, satellites and navigation systems. While historical events such as the 1859 Carrington Event and the storms in 2024 provide valuable data, these 'once-in-a-century' scenarios continue to push the boundaries of our current operational frameworks. This session will evaluate the state of physics-based and machine learning forecasting models to bridge the gap between scientific theory and infrastructure resilience.
Key objectives:
- Evaluate the reliability and limitations of current monitoring tools.
- Identify the data and modelling gaps needed to improve extreme event forecasting.
- Define worst-case scenarios and their socio-economic impacts.
- Develop concrete mitigation strategies and cross-sector communication channels.
We invite submissions from academia and industry focusing on the impact of extreme events on the magnetosphere, ionosphere and thermosphere.
Conveners: Rungployphan Kieokaew (IRAP, France), Simone Di Matteo (CUA & NASA, USA), Judith de Patoul (ROB, Belgium), Maxime Grandin (FMI, Finland), Alexi Glover (ESA).
Submit your abstract: https://www.egu26.eu/session/57156
3. Abstract submission: Advertisement for two sessions at EGU 2026, abstract deadline: 15 January 2026, 13:00 CET.
From: Giulia Cozzani, LPC2E, Orléans, France, <giulia.cozzani at cnrs-orleans.fr>
Subject: Advertisement for two sessions at EGU 2026.
Please consider submitting an abstract to our session at the EGU General Assembly 2026:
Turbulence in Space Plasmas: Structures, Waves, and Dissipation
https://www.egu26.eu/session/55797
The session is dedicated to advancing our understanding of plasma turbulence across diverse environments, from the solar wind and planetary magnetospheres to astrophysical systems. We welcome contributions spanning observational, theoretical, numerical, and laboratory approaches, with a focus on open questions regarding coherent structures, wave-particle interactions, dissipation mechanisms, and cross-scale energy transport.
We encourage submissions related to space science, astrophysical plasmas, near-Earth processes, heliospheric physics, turbulence theory, high-performance numerical simulations, and innovative satellite data analysis. In particular, we seek contributions utilizing data from current and past missions - including Wind, Cluster, MMS, STEREO, THEMIS, Van Allen Probes, and DSCOVR - with a special emphasis on new findings from Parker Solar Probe and Solar Orbiter.
Key Information:
Meeting: EGU General Assembly 2026, 3–8 May 2026 (Vienna & Online)
Abstract Deadline: 15 January 2026, 13:00 CET
Convener: Sergio Servidio (University of Calabria, Italy)
Co-convener: Luca Sorriso-Valvo (Institute for Plasma Science and Technology - CNR, Italy), Julia Stawarz (Northumbria University, United Kingdom), Giulia Cozzani (LPC2E, France), Louis Richard (Swedish Institute of Space Physics, Sweden)
ST2.2 – Unveiling plasma energization and energy transport in Geospace via multiscale observations
https://www.egu26.eu/session/57149, Co-organized by NP3/PS4.
This session focuses on understanding how plasma is energized and how energy is transported across scales in the Earth’s Magnetospheric System. Key processes include shock dynamics, magnetic reconnection, turbulence, wave-particle interactions, and plasma jets. While past missions such as Cluster, MMS, and THEMIS have revealed important single-scale physics, fully capturing cross-scale coupling requires true multi-scale observations. The multi-scale approach is central to the Plasma Observatory (PMO) mission concept.
We welcome contributions from observations, simulations, theory, and instrumentation, as well as studies linking in-situ, remote-sensing, and ground-based measurements. Submissions highlighting multi-scale or cross-scale dynamics are particularly encouraged.
Key Information:
Meeting: EGU General Assembly 2026, 3–8 May 2026 (Vienna & Online)
Abstract Deadline: 15 January 2026, 13:00 CET
Conveners: Matthew Taylor (ESA, Netherlands), Oreste Pezzi (ISTP-CNR, Italy), Giulia Cozzani (LPC2E, France), Markku Alho (University of Helsinki, Finland)
4. Call for Abstracts: Call for abstracts EGU 2026 session ST4.6 Modelling and observations of the near-Earth space weather environment, deadline: January 15, 2026, 13:00 CET.
From: Jorge Amaya, European Space Agency, <jorgeluis.amaya at gmail.com>
Subject: Call for abstracts EGU 2026 session ST4.6 Modelling and observations of the near-Earth space weather environment.
Conveners: Jorge Amaya (ESA), Melanie Heil (ESA), Antoine Resseguier (IRAP/CNRS)
Link: https://www.egu26.eu/session/57151
Deadline: January 15, 2026, 13:00 CET
We would like to invite all entities and research groups working of the development of instruments and computer models used for the monitoring, analysis, and forecasting of the near Earth environment, to submit an abstract to this comprehensive EGU session, presenting their latest advancements and concepts. We will highlight the unique capabilities and features of the latest instruments dedicated to monitoring the ionosphere, the thermosphere, the aurora, and the radiation belts, and their interactions. This session will also feature presentations on computer models that transform complex data into valuable understanding, enabling us to anticipate and address the challenges posed by space weather. Join us to be inspired by opportunities for scientific collaboration and see how these innovations support operational monitoring for end users, ultimately helping to safeguard our technology and society.
5. Call for Abstracts: Invitation to submit to EGU 2026 Session ST1.6: Observing and modelling coronal mass ejections from the Sun to the heliosphere, abstract submission deadline is Thursday, 15 January 2026, 13:00 CET.
From: Greta Cappello, University of Graz, <greta.cappello at uni-graz.at>
Subject: Call for Abstracts: Invitation to submit to EGU 2026 Session ST1.6: Observing and modelling coronal mass ejections from the Sun to the heliosphere, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
EGU 2026 abstract submission is now open and we welcome any CME-related submissions involving remote sensing/in situ observations, multi-spacecraft studies, modeling efforts, or mission concepts to our session:
ST1.6: Observing and modelling coronal mass ejections from the Sun to the heliosphere: https://www.egu26.eu/session/57164
Confirmed invited speakers include:
Eleanna Asvestari: Data driven CME modelling
Alessandro Liberatore: CMEs observed with PROBA-3/ASPIICS and Solar Orbiter/Metis
Abstract submission deadline is Thursday, 15 January 2026, 13:00 CET. If you would like to submit an abstract, you can do so via this link:
https://meetingorganizer.copernicus.org/EGU26/abstractsubmission/57164
Co-conveners: Emma Davies, Erika Palmerio, David Barnes, and Greta Cappello
6. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.7 –Global magnetospheric-ionospheric dynamics in simulations and observations, the deadline for the abstract submissions is 15 January 2026, 13:00 CET.
From: Andrey Samsonov, University College London, <a.samsonov at ucl.ac.uk>
Subject: Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.7 –Global magnetospheric-ionospheric dynamics in simulations and observations, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
We would like to draw your attention and invite you to submit an abstract to the ST2.7 session "Global magnetospheric-ionospheric dynamics in simulations and observations" in the ST2-Magnetosphere programme group of the European Geosciences Union (EGU) General Assembly 2026. The General Assembly 2026 of the EGU will be held 3-8 May 2026, in Vienna and online.
Session page: https://meetingorganizer.copernicus.org/EGU26/session/57138
Please note that the deadline for the abstract submissions is 15 January 2026, 13:00 CET.
Session description: Large-scale dynamic processes in different regions are closely interconnected, and the coupled magnetosphere-ionosphere-thermosphere (MIT) should therefore be considered as a global system. The state of the MIT system is controlled mainly by solar wind conditions. The interplanetary magnetic field (IMF) and solar wind velocity govern the energy input, but solar wind properties change when plasma moves through the bow shock and magnetosheath. The magnetic reconnection rate at the dayside magnetopause depends on parameters in the magnetosheath and magnetosphere rather than directly on solar wind conditions. Once dayside reconnection starts, magnetic flux accumulates in the magnetotail lobes, resulting in substorms or steady magnetospheric convection. Reconnection in the magnetotail injects thermal and energetic particles into the inner magnetosphere and ionosphere, and ionospheric particles can escape along magnetic field lines into the magnetosphere. The Kelvin-Helmholtz instability provides another important mechanism to transfer energy from the solar wind into the magnetosphere.
These global dynamics can be studied with increasingly sophisticated numerical simulations (MHD, hybrid, or fully kinetic), with empirical and semi-empirical models, or by using a variety of observations, including in situ spacecraft observations and ground-based measurements. Past and future global imaging missions (e.g., SMILE and GEO-X) complete this picture, providing large-scale snapshots. Accurate modelling of global processes is essential for successful space weather predictions, but sometimes model predictions differ largely even for typical solar wind conditions. We welcome work presenting results on the global dynamics of the MIT system on Earth, as well as on other planets.
Convener: Andrey Samsonov, Co-conveners: Yulia Bogdanova, John Coxon, Bayane Michotte de Welle, and Venla Koikkalainen
7. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.3 -- Magnetic reconnection and associated multi-scale coupling in the collisionless environments, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
From: Seiji Zenitani, Space Research Institute, AUSTRIA, <seiji.zenitani at oeaw.ac.at>
Subject: Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.3 -- Magnetic reconnection and associated multi-scale coupling in the collisionless environments, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
We invite submissions to the EGU 2026 session ST2.3 on magnetic reconnection. Submissions on spacecraft measurements, theoretical analysis, numerical simulations, laboratory experiments, and possibly other aspects on magnetic reconnection are welcome. The full session description is available at https://meetingorganizer.copernicus.org/EGU26/session/57152
Conveners: Seiji Zenitani, Rongsheng Wang, Maria Elena Innocenti, Wenya Li, Kyoung-Joo (Joo) Hwang
8. Call for Abstracts: Invitation to submit abstracts to EGU 2026 Session ST2.9 - Inner Magnetosphere, Ionosphere, and Atmosphere Coupling, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
From: Dedong Wang, GFZ Helmholtz Center for Geosciences, <dedong at gfz.com>
Subject: Invitation to submit to EGU 2026 Session ST2.9: Inner Magnetosphere, Ionosphere, and Atmosphere Coupling.
We welcome theoretical, modelling, and observational contributions on the dynamics of inner magnetospheres at Earth and other planets, including magnetosphere–ionosphere coupling and responses to solar wind disturbances. Relevant datasets include MMS, THEMIS, Van Allen Probes, Arase, Cluster, LEO satellites, CubeSats, Juno, SuperDARN, magnetometers, optical imagers, incoherent scatter radars, and ground-based VLF measurements. The conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
The full session description is available at https://meetingorganizer.copernicus.org/EGU26/session/57139
Convener: Dedong Wang | Co-conveners: Hilde Nesse, Ondrej Santolik, Yuequn Lou, Alwin Roy
9. Call for Abstracts: Invitation to submit to EGU 2026 Session ST3.3 – Modeling the Interconnected Thermosphere, Ionosphere, Plasmasphere and Magnetosphere, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
From: Sadaf Shahsavani, GFZ Helmholtz Center for Geosciences, <sadaf.shahsavani at gfz.de>
Subject: Invitation to submit to EGU 2026 Session ST3.3 – Modeling the Interconnected Thermosphere, Ionosphere, Plasmasphere and Magnetosphere.
We especially welcome contributions on:
- Data-driven modeling and global-scale interactions between these regions
- Combination of multiple measurement techniques, such as low Earth orbit (LEO) satellites or remote sensing.
- Identification and incorporation of external drivers for accurate modeling of the response of the near-Earth environment to space weather.
- Innovative approaches that include data assimilation, machine learning, empirical or numerical modeling.
The conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
The full session description is available at https://meetingorganizer.copernicus.org/EGU26/session/58177
Convener: Lucas Schreiter | Co-conveners: Armin Corbin, Sadaf Shahsavani, Ehsan Forootan, Randa Natraš
10. Call for Abstracts: Invitation to submit to EGU 2026 Session ST2.4 – Wave-particle interactions, the conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
From: Mirek Hanzelka, <mirekhanzelka at gmail.com>
Subject: Invitation to submit to EGU 2026 Session ST2.4 – Wave-particle interactions.
We invite submissions to the EGU 2026 session ST2.4: Regimes of wave-particle interactions in terrestrial and planetary magnetospheres and the solar wind. The conference will take place in Vienna, Austria, from 3 to 8 May, 2026.
The full session description is available at https://meetingorganizer.copernicus.org/EGU26/session/57140
Short description: This session focuses on wave-particle interactions in collisionless plasmas and their role in wave generation, damping, and particle scattering in the radiation belts and beyond. It gathers theorists, data analysts, and modelers to advance frameworks that integrate nonlinear and non-resonant effects into diffusion-based plasma models.
11. SHIELD Webinar Invitation: SHIELD Webinar Featuring Alan Stern, on Friday, February 13th at Noon ET.
From: Nick Gross, Boston University, <gross at bu.edu>
Subject: SHIELD Webinar Featuring Alan Stern.
Join us for the next SHIELD Webinar where we will host
Alan Stern speaking on “My Career in Planetary Science and Exploration”, Friday, February 13th at Noon ETRegister at https://shielddrivecenter.com/shield-webinars/
Dr. Alan Stern is an aerospace executive, flown suborbital astronaut, and planetary scientist with experience on 30 space mission teams. Among those are the New Horizons mission which has explored Pluto and the Kuiper Belt—the farthest exploration of worlds in History.
In 2007 and 2008 Dr. Stern directed NASA’s entire science program. He currently serves as an executive in the Southwest Research Institute (SwRI) and serves on the board of several space science organizations and companies. He is the father of three grown children and resides near Boulder, Colorado.
12. Call for Abstracts: COSPAR PSW.6 (2026), deadline: February 13.
From: Claudio Corti, CCMC, <corti at hawaii.edu>
Subject: Abstract Call: COSPAR PSW.6 (2026), deadline: February 13.
We would like to draw your attention to COSPAR 2026 Session PSW.6: What are the critical parameters required to predict solar energetic particle events?
https://www.cospar-assembly.org/admin/session_cospar.php?session=1549
This session aims to get at the heart of the observations and physical processes that are critical to enable accurate SEP predictions: Numerous solar energetic particle (SEP) forecasting models have been developed with a wide variety of approaches. Recent validation efforts, e.g. SEPVAL and the SEP Scoreboards, have demonstrated that SEP models show some skill at predicting SEP events on average but that models are not yet able to predict the characteristics of any given individual event with high fidelity. In other words, the current state-of-the-art tends to predict the average statistical SEP event associated with a certain set of triggers, whereas end-users need a prediction for THIS SEP event. This session asks which key physical parameters determine the unique characteristics for each SEP event? How do we capture the range of possibilities for a specific SEP event - likely, worst-case, and best-case outcomes? Which existing observations may improve predictive power but are not yet utilized in any schemes? How do solar wind structures in the inner heliosphere impact SEP outcomes? Are there certain conditions that are always or only present during extreme SEP events? What do human forecasters use to predict SEPs? We encourage talks about the predictive nature (or lack thereof) of available observations or physical conditions, as well as sensitivity studies of SEP forecasting models.
The deadline for abstract submission is February 13: https://www.cospar-assembly.org
13. Invitation: The SCOSTEP's 16th Quadrennial Solar-Terrestrial Physics Symposium, deadline of abstract submission: 26 January 2026 (extended from 10 January 2026).
From: Rumi Nakamura, IWF, OEAW, <rumi.nakamura at oeaw.ac.at>
Subject: The SCOSTEP's 16th Quadrennial Solar-Terrestrial Physics Symposium.
We invite your participation at the SCOSTEP's 16th Quadrennial Solar-Terrestrial Physics Symposium (STP 6) will be held on 1-5 June 2026 (school on 30-31 May 2026) at Makedonia Palace Hotel, Thessaloniki, Greece. Website: https://www.stp2026.org/
Deadline of abstract submission: 26 January 2026 (extended from 10 January 2026)
STP-16 aims to gather eminent scientists from solar, magnetospheric, ionospheric, and atmospheric physics communities to discuss and deliberate on the cutting-edge sciences pertaining to solar-terrestrial physics (STP), especially the cross-scale coupling processes as a focus area, as a kick-off activity of the SCOSTEP’s new program. COURSE - Cross-Scale Coupling Processes in the Solar-Terrestrial System in 2026-2030.
Science Organizing Committee of STP-16
Scientific Committee on Solar-Terrestrial Physics (SCOSTEP) https://scostep.org/
14. Call for Proposals: Dissemination request - ISSI International Team Call for Proposals (2026), Proposal deadline is 13 March 2026.
From: Sabina Raducan, International Space Science Institute (ISSI), <sabina.raducan at issibern.ch>
Subject: Dissemination request - ISSI International Team Call for Proposals (2026).
I am writing to kindly ask for your support in disseminating the ISSI International Team Call for Proposals in Space and Earth Sciences, jointly issued by the International Space Science Institute (ISSI) in Bern and ISSI-BJ in Beijing.
ISSI/ISSI-BJ invite proposals to establish International Teams conducting collaborative research in the Space and Earth Sciences at the respective ISSI and ISSI-BJ meeting facilities. It is open to scientists worldwide, regardless of nationality or institutional affiliation, who are actively engaged in research in Astrophysics, Heliophysics, Planetary Science, or Earth Sciences.
To be eligible, projects must make use of data from space missions. Where this adds scientific value, projects may also draw on complementary ground-based data and/or theoretical modelling.
ISSI and ISSI-BJ provide an open, interactive research environment, high-quality facilities, and cover local expenses for meeting participants through accommodation and per diem support.
Proposal deadline is 13 March 2026.
Please find the full text of the Call for Proposals here: http://www.issibern.ch/docs/ISSI_ISSI-BJ_annual_call2026.pdf
15. Call for abstracts: 46th COSPAR Scientific Assembly, the abstract deadline is 13 February 2026.
From: Nicole Vilmer, LIRA-Paris Observatory-PSL Research University- Chair of COSPAR CommissionD, <nicole.vilmer at obspm.fr>
Subject: 46th COSPAR Scientific Assembly: Call for abstracts.
The 46th COSPAR Scientific Assembly will take place in Florence, Italy, from 1–9 August 2026.
Submission of abstracts for the 46th Scientific Assembly of the Committee on Space Research (COSPAR) is open and the abstract deadline is 13 February 2026. You can find the relevant information on the following site: https://www.cospar-assembly.org/assembly.php
Several sessions are organized by Commission D on topics relevant to solar and heliospheric physics.
D1.1 Transport and Acceleration of Energetic Particles in the Heliosphere, the Interstellar Medium, and Astrospheres
D1.2 Science with Interstellar Mapping and Acceleration Probe (IMAP)
D1.3 Solar Energetic Particle Events throughout the Solar System: Understanding and Forecasting
D2.1/E3.1 Off-the-Sun-Earth-Line (OSEL) missions for a 3D view of the Sun and Heliosphere
D2.2/E3.2 Heliophysics Multi-Messenger Era: from Exploration to Paradigm Shifting Discoveries
D2.3/E3.3 Magneto-plasma Structures, Streams and Flows in the Heliosphere
D2.4/E3.4 Magnetic Reconnection in a Turbulent Plasma from the Sun to the Heliosphere
D2.5/E3.5 Stellar Forcing of Planetary and Exoplanetary Space Environments
D2.6/E3.6 The Multifaceted Solar Wind: From its Origins on the Sun to Earth
16. Webinar: Solar Orbiter community building webinar #1 (2026), take place on Wednesday 4 February 2026 (14:00 - 14:30 CET).
From: Miho Janvier, ESA, <miho.janvier at esa.int>
Subject: Solar Orbiter community building webinar #1 (2026).
The first of the Solar Orbiter community building webinars (season 2, hosted by Dr Jack Jenkins) will take place on **Wednesday 4 February 2026 (14:00 - 14:30 CET).**
This webinar, titled “The high latitude phase of the Solar Orbiter mission.”, will be presented by Dr David Williams (ESA/ESAC, Spain).
As a reminder, the aim of these webinars is to provide news and insights on Solar Orbiter science and science operations to the wider solar and space physics communities.
Registration for the webinar link can be found here:
https://esait.webex.com/weblink/register/r7b37daae8afa5e704112041375f1e33c
Information on future webinars can be found here: https://www.cosmos.esa.int/web/solar-orbiter/webinars
------------------------------------------------------------------------------------------------------------------ ------