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<p class="elementToProof" style="margin-top: 0px; margin-bottom: 0px;"><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">URSI AT-RASC 2024 Commission H Session Announcement</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">The triennial URSI Atlantic Radio Science Conference (URSI AT-RASC) is one of the URSI flagship conferences, alongside the URSI General Assembly and Scientific
Symposium (GASS) and the Asia-Pacific Radio Science Conference (AP-RASC).</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">The 4th URSI AT-RASC will be held May 19-24, 2024, in Gran Canaria, Spain, as a fully in-person conference with only on-site presentations. The conference
will have a series of convened and open sessions within the domains covered by all ten Commissions of URSI. Abstract submissions are now open, and the submission deadline is January 20, 2024.</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">Below you will find a brief overview of the sessions led by Commission H; the complete list of sessions and their descriptions are available here:</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(17, 85, 204);"><u><br>
</u><a href="https://www.atrasc.com/papersubmission.php" id="OWA96469883-9c9d-5dbe-5c27-55b45182532e" class="OWAAutoLink" style="text-decoration: none; margin-top: 0px; margin-bottom: 0px; color: rgb(17, 85, 204);">https://www.atrasc.com/papersubmission.php</a></span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);"><u>.</u></span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H01: Open Session</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">In one sentence: This session solicits papers on all aspects of waves in space and laboratory plasmas that do not easily fit into the other sessions within
Commission H for this URSI meeting. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">Conveners: Craig Rodger, Robert Marshall</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H02: Plasma waves, wave-particle interactions, and their multifold effects on the radiation belts</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session invites studies
that advance our current understanding of wave-particle interactions and their role in radiation belt dynamics from observational, theoretical, and numerical points of view. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: David Hartley, Ondrej Santolik, Vania
Jordanova, Yoshizumi Miyoshi</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H03: Machine learning techniques and applications to wave-particle interaction processes in space plasmas</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session will focus on applications
of machine learning techniques to wave-particle interactions through the analysis of observational data, large-scale simulation data, or the fusion of observational and simulation data.</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Drew Turner, Savvas Raptis, David Malaspina</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H04: Recent advances in geospace research from multi-point observations</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session solicits new findings
and advances in geospace research combining the datasets from various satellites missions as well as ground-based networks and numerical simulations.</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Jyrki Manninen, Jean-Francois Ripoll,
Yoshiya Kasahara</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H05: Radio diagnostics of space weather plasma processes </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session is open to contributions
relevant to theoretical models, e.g. of solar radio bursts and ionospheric emissions, radio signatures’ interpretation, and observation techniques, in the framework of both Space Weather science and Space Weather operations. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Mauro Messerotti, Natchimuthuk Gopalswamy</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H06: Computer simulations in space plasmas </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session solicits state-of-the-art
simulation advances and results related to space plasma physics. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Esa Kallio (Aalto University, Finland),
Yohei Miyake (Kobe University) </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H07: Analysis of natural boundary layers in terrestrial and planetary environments: Macro/micro scale kinetic approaches</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session solicits contributions
related to boundary layers in magnetospheric, ionospheric and space plasma physics, including (i) collisionless shocks and/or foreshocks, (ii) the magnetopause, (iii) plasma sheet currents, (iv) nearby/far magnetotail dynamics (including substorms), (v) plasmapause,
(vi) potential drops in the ionosphere and cusp dynamics, (vii) basic particle acceleration processes, (viii) impact of transients carried by the solar wind on these interfaces and (ix) dynamics of interfaces in active space experiments. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Hui Zhang, Philippe Escoubet, Xóchitl
Blanco Cano, David Sibeck</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H08: Turbulence and Instabilities in Space Plasmas </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: The session welcomes contributions
on the use of radio observations to determine the nature of density and velocity fluctuations remotely in the solar wind, alongside work on the theory, numerical modeling, and in situ observations of turbulence and instabilities. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Alexander Pitňa, Owen Wyn Roberts,
Julia Stawarz, Domenico Trotta, Gary Zank</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">H09: Tribute to Craig Kletzing - his fascination with plasma waves and the upcoming TRACERS mission </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session involves a single
invited presentation by Professor David Miles, given in tribute to Professor Craig Kletzing and his many contributions to experimental space plasma physics.</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Ondřej Santolík, David Hartley</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);"><u>Joint Sessions Led by Commission H: </u></span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">HG01: Active Experiments in Space and Laboratory Plasmas </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session will cover recent
advances in active experiments in space and in the laboratory that seek to advance and test theories or build diagnostic or predictive capabilities. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Robert Moore, Mark Golkowski</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">HG02: Observations of near- Earth space from Small Satellites and Suborbital Platforms </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session solicits contributions
describing recent or upcoming small satellite, sounding rocket, or high-altitude balloon missions aimed at addressing science goals in the near-Earth space environment through remote sensing and/or in-situ measurements. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Robert Marshall, Bruce Fritz, David
Malaspina</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">HGE01: Atmospheric, ionospheric, magnetospheric, and high energy effects of lightning discharges </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session solicits contributions
that advance knowledge in the areas of the global atmospheric electric circuit, lightning physics, transient luminous events, energetic radiation, relativistic particles, and their impact on the Earth's atmosphere, ionosphere and magnetosphere. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Ivana Kolmašová, Martin Fullekrug,
Ningyu Liu</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">HGE02: Meet the HGE Experts - Presentations </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: In this session, we invite a
panel of renowned researchers to give their opinions on how the research field has evolved since they started their careers, and what are key questions for the future of space physics. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: František Němec, Bruce Fritz, Riccardo
Trinchero</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">HGE03: Meet the HGE Experts - Panel Discussion </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Following the panel session of
‘Meet the Experts’ for commissions HGE, this Q&A session will give the opportunity to early-career scientists to ask questions to our experts, either about their scientific research or their career paths and experience. </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Ivana Kolmašová, Martin Fullekrug,
Ningyu Liu</span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">HJ01: Radio emission from the Sun, Heliosphere, and Planets </span></p>
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<span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">In one sentence</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: This session solicits contributions
that report on recent observations of solar, heliospheric and planetary radio emissions, including coordinated multi-point observations from ground radio telescopes and spacecraft plasma/wave experiments. </span></p>
<div class="elementToProof"><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 700; color: rgb(0, 0, 0);">Conveners</span><span style="font-family: Arial, sans-serif; font-size: 11pt; font-weight: 400; color: rgb(0, 0, 0);">: Pietro
Zucca, Patrick Galopeau, Natchimuthuk Gopalswamy, Yihua Yan</span></div>
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