› Cluster Mission status - Philippe Escoubet, ESTEC/ESA
09:10-09:25 (15min)
› Goetz Paschmann (1939-2023), Scientist – Colleague – Friend - Gerhard Haerendel, Max Planck Institute for Extraterrestrial Physics (INVITED)
09:25-09:45 (20min)
› Magnetic reconnection observed with Cluster - Andris Vaivads, KTH Royal Institute of Technology, Stockholm, Ventspils University of Applied Sciences (INVITED)
09:45-10:05 (20min)
› Charged particle acceleration in the magnetotail: Cluster/RAPID insights - Elena Kronberg, Ludwig-Maximilians-Universität München (INVITED)
10:05-10:25 (20min)
› Impact of the Kelvin-Helmholtz instability on the Space Weather Driving of the Earth's Magnetosphere: Discoveries from Cluster Mission Fostering Rapid Progress for More Recent Missions. - Katariina Nykyri, Embry-Riddle Aeronautical University (INVITED)
10:25-10:45 (20min)
› Nicole Cornilleau-Wehrlin: Woman Space Scientist. Her Legacy to Cluster and Beyond - Patrick Canu, Laboratoire de Physique des Plasmas (INVITED)
11:25-11:45 (20min)
› Turbulence in space plasmas and multi-point techniques: Cluster legacy - Olga Alexandrova, LIRA (INVITED)
11:45-12:05 (20min)
› Electrostatic Solitary Waves in the Near-Earth Plasma Environment - Cluster Observations - Daniel Graham, Swedish Institute of Space Physics (INVITED)
12:05-12:25 (20min)
› Highlights of the Cluster Ion Spectrometry (CIS) experiment, following 24 years of successful operation - Iannis Dandouras, Institut de recherche en astrophysique et planétologie (INVITED)
12:25-12:45 (20min)
› Hugo Alleyne: 'treat everyone as if they were your own' - Keith Yearby, University of Sheffield (INVITED)
13:45-14:05 (20min)
› Shocks observations with Cluster with emphasis on particle energization - Andrew Dimmock, Swedish Institute of Space Physics, Uppsala
14:05-14:25 (20min)
› Foreshock waves and transients: a review of advances in the Cluster era - Lucile Turc, Department of Physics, University of Helsinki
14:25-14:45 (20min)
› Curlometer and gradient techniques - Malcolm Dunlop, RAL Space, STFC-UKRI, Beihang University
14:45-15:05 (20min)
› Magnetic nulls and turbulent reconnection as revealed by the Cluster mission - Huishan Fu, Beihang University
15:05-15:25 (20min)
› Klaus Torkar: a career devoted to control the electric potential of spacecraft - C. Philippe Escoubet, European Space Research and Technology Centre
16:05-16:25 (20min)
› Cluster PEACE highlights - Andrew Fazakerley, Mullard Space Science Laboratory (INVITED)
16:25-16:45 (20min)
› Access of Ionospheric Outflow to the Magnetotail and Inner Magnetosphere - Lynn Kistler, University of New Hampshire (INVITED ONLINE)
16:45-17:05 (20min)
› Fluxgate magnetometer calibration trends during the Cluster mission 2021-2024 - Chris Carr, Imperial College - Leah-Nani Alconcel, University of Birmingham [Birmingham] (INVITED)
17:05-17:25 (20min)
› Hermann Opgenoorth: His Legacy for Multi-Instrument, Multi-Point Observations of Space Plasmas - Mark Lester, University of Leicester (INVITED ONLINE)
17:25-17:45 (20min)
› From multi-point to multi-scale plasma physics in the Magnetospheric System: Plasma Observatory as next logical step after Cluster and MMS - Rumi Nakamura, Space Research Institute, Austrian Academy of Sciences (INVITED)
17:45-18:15 (30min)
› Validating a 3D ULF wave model Using Cluster and Ground-based Observations of an FLR event Triggered by a Foreshock Transient - Alexander Degeling, Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai
18:15-19:45 (1h30)
› Energization of Outflowing O+ by Double‐Pickup in Earthward Plasma Jets From Lobe Reconnection and in Magnetosheath Flow - Haruto Koike, University of Kyoto
18:15-19:45 (1h30)
› Automatic Classification of Plasma Regions and Detection of Plasma Jets in Near-Earth Space Using Supervised Machine Learning - Soboh Alqeeq, Laboratoire de Physique des Plasmas
18:15-19:45 (1h30)
› Spatial Distributions of Energetic Electrons and Energetic Ions in the Tail Reconnection Region: Cluster Observations vs. PIC Simulations - Shiyong Huang, School of Earth and Space Science and Technology, Wuhan University
18:15-19:45 (1h30)
› The Cluster GRMB (Geospace Region and Magnetospheric Boundary) dataset applied to case and statistical studies: “Double plasmasphere” event and 3D visualization of the magnetosphere and solar wind - Fabien Darrouzet, Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Brussels
18:15-19:45 (1h30)
› Multi-spacecraft analysis of interplanetary discontinuities at 1 AU -
18:15-19:45 (1h30)
› Electrostatic Solitary Waves: Can they accelerate the solar wind? - Chadi Salem, Space Sciences Laboratory, University of California Berkeley
18:15-19:45 (1h30)
› Electric currents and turbulent dynamics in the magnetosphere/ionosphere system - Péter Kovács, HUN-REN Wigner Research Centre for Physics [Budapest]
18:15-19:45 (1h30)
› Exploring Plasma Observatory Orbits via Analogue Trajectories and Solar Activity: Evidence of Kelvin–Helmholtz and Tearing Mode Instabilities - Lorenzo Biasiotti, INAF - Osservatorio Astronomico di Trieste
18:15-19:45 (1h30)
› Intermittent reconnection in the magnetotail - Cecilia Norgren, Swedish Institute of Space Physics [Uppsala / Kiruna], University of Bergen
18:15-19:45 (1h30)
› Use of Twenty Years CLUSTER FGM Data to Observe the Mean Behaviour of the Magnetic Field and Current Density of Earth's Magnetosphere - Patrick Robert, Laboratoire de Physique des Plasmas
18:15-19:45 (1h30)
› Cluster observations of foreshock waves: utilising all 23 years of data -
18:15-19:45 (1h30)
› Current sheet thinning in turbulent reconnection - Emiliya Yordanova, Swedish Institute of Space Physics, Uppsala
18:15-19:45 (1h30)
› Exploring Scale-Dependent Energy Dynamics in Solar Wind Simulations - Christian Vasconez, Departamento de Fisica, Escuela Politecnica Nacional
18:15-19:45 (1h30)
› Chorus wave propagation ducted by ultralow frequency wave: event analysis and ray-tracing simulation - Kohki Tachi, Graduate School of Science Department of Geophysics, Tohoku University, Faculty of Mathematics and Physics, Charles University, Institute of Atmospheric Physics, Czech Academy of Sciences
18:15-19:45 (1h30)
› Localization of EMIC waves observed by the Cluster satellites in geospace with the publicly available GRMB (Geospace Region and Magnetospheric Boundary) dataset -
18:15-19:45 (1h30)
› Field-Aligned Ion Beams in the Terrestrial Foreshock: Insights from Cluster Multi-Point Observations - Karim Meziane, University of New Brusnwick
18:15-19:45 (1h30)
› Suprathermal Electron Acceleration Comparison of the Venusian and Terrestrial Bow Shocks - Ulf Martin Lindberg, Queen Mary University of London
18:15-19:45 (1h30)
› Cluster and THEMIS: Cross-Calibration of Energetic Electron Flux Measurements - Elena Kronberg, Ludwig Maximilian University [Munich] = Ludwig Maximilians Universität München
18:15-19:45 (1h30)
› Fluxgate magnetometer Extended Mode dataset in the Cluster Science Archive - Chris Carr, Imperial College - Leah-Nani Alconcel, University of Birmingham [Birmingham]
18:15-19:45 (1h30)
› STABILITY AND TRANSPORT IN THE TURBLENT PLASMA SHEET - Marina Stepanova, UNIVERSIDAD DE SANTIAGO DE CHILE
18:15-19:45 (1h30)
› Unique opportunities to study the magnetopause with Cluster - Niklas Grimmich, Institute for Geophysics and extraterrestrial Physics, TU Braunschweig
18:15-19:45 (1h30)
› Evolution of Electron-to-Ion Temperature Ratio of Cold Plasma in the Lobes - Kun Li, Sun Yat-Sen University [Guangzhou]
18:15-19:45 (1h30)
› An improved method to detect the low-energy ion flows in the near-Earth polar cap regions - Kun Li, Sun Yat-Sen University [Guangzhou]
18:15-19:45 (1h30)
› Features of Field Aligned Electrons in Polar Region: Cluster Observation - Jiankui Shi, National Space Science Center [Beijing], ESA - ESTEC (Netherlands), STFC Rutherford Appleton Laboratory, Mullard Space Science Laboratory, Department of Physics [Imperial College London]
18:15-19:45 (1h30)
› Waves instrument suite for Plasma Observatory - Yuri Khotyaintsev, Swedish Institute of Space Physics [Uppsala]
13:40-14:00 (20min)
› Electric Field Dipole Antenna (EFI –ADA) - Marek Morawski, Space Research Centre PAS (ONLINE)
14:00-14:20 (20min)
› The Plasma Observatory MAG Instrument - Evgeny Panov, Space Research Institute of Austrian Academy of Sciences - Gerlinde Timmermann, Technische Universität Braunschweig = Technical University of Braunschweig [Braunschweig]
14:20-14:40 (20min)
› The SCM for Plasma Observatory - Olivier Le Contel, Laboratoire de Physique des Plasmas
14:40-15:00 (20min)
› BOX-P unit for PMO mission - Hanna Rothkaehl, Space Research Centre PAS
15:40-16:00 (20min)
› The ion and Electron Plasma Camera for the Plasma Observatory mission - Matthieu Berthomier, Laboratoire de Physique des Plasmas
16:00-16:20 (20min)
› The Ion Mass Composition Analyser for the ESA Plasma Observatory mission - Maria Federica Marcucci, Istituto di Astrofisica e Planetologia Spaziali - INAF
16:20-16:40 (20min)
› The Energetic Particle Experiment on Plasma Observatory - Malcolm Dunlop, RAL Space, STFC-UKRI, Beihang University
16:40-17:00 (20min)
› EMC challenges of the Plasma Observatory mission - Zoltan Kiss, ESA (INVITED ONLINE)
17:00-17:20 (20min)
› ESA charging and Payload performance activities regarding PMO - Fredrik Johansson, ESA - ESTEC (INVITED)
17:20-17:40 (20min)
PMO science: How are particles energized in near-Earth space plasmas ?
Auditorium
D. Trotta & Y. Khotyaintsev
› Mechanisms for ion and electron energization at shocks and foreshock transients - Heli Hietala, Department of Physics and Astronomy, Queen Mary University of London (INVITED)
16:00-16:30 (30min)
› Adiabatic and Non‐Adiabatic Electron Heating at Quasi‐ Perpendicular Collisionless Shocks - Ahmad Lalti, Northumbria University (INVITED ONLINE)
16:30-16:50 (20min)
› The interaction of plasma turbulence and perpendicular shock waves in hybrid simulations - Laura Vuorinen, Department of Physics and Astronomy, Queen Mary University of London (INVITED)
16:50-17:10 (20min)
› Particle transport around interplanetary shock waves. - Silvia Perri, Dipartimento di Fisica, Università della Calabria (INVITED)
17:10-17:30 (20min)
› Compound electron acceleration at planetary foreshocks - Xiaofei Shi, University of California, Los Angeles (INVITED ONLINE)
17:30-17:50 (20min)
› Multi-scale mechanisms of charged particle acceleration in magnetotail plasma jets - Anton Artemyev, Department of Earth, Planetary and Space Sciences, UCLA (INVITED ONLINE)
17:50-18:20 (30min)
› Magnetosheath Jets and Foreshock Transients Contribution to Particle Energization at Collisionless Shocks - Savvas Raptis, Applied Physics Laboratory, The Johns Hopkins University (INVITED ONLINE)
18:20-18:40 (20min)
› Toward Multi-Spacecraft Exploration of Jet–Turbulence Coupling in the Magnetosheath - Florian Koller, Department of Physics and Astronomy, Queen Mary University of London, London, UK
18:40-18:55 (15min)
› Multipoint Measurements for Analysis of Physical Fields - Dorota Przepiórka-Skup, Space Research Centre of the Polish Academy of Sciences
18:55-20:30 (1h35)
› Simulations of Plasma Observatory's Energetic Particle Experiment - Hannes Ebeling, Kiel University, Institute for Experimental and Applied Physics, Kiel, Germany - Svea Jürgensen, Kiel University, Institute for Experimental and Applied Physics, Kiel, Germany
18:55-20:30 (1h35)
› Driving of Large Amplitude Compressional ULF waves by an IMF Southward Turning and Solar Wind Pressure Pulses - Chiara Lazzeri, Mullard Space Science Laboratory
18:55-20:30 (1h35)
› Turbulence-Driven Magnetic Reconnection and Turbulent Heating in Earth's Magnetoseath - Julia Stawarz, Northumbria University [Newcastle]
18:55-20:30 (1h35)
› Towards Multi-Scale Magnetospheric Simulations: Adaptive Mesh and Model Refinement with PHARE - Ulysse Caromel, LPP
18:55-20:30 (1h35)
› Scale-dependent Skewness and Kurtosis in Kinetic Plasmas and Magnetohydrodynamic Systems - Jiaming Wang, University of Delaware [Newark]
18:55-20:30 (1h35)
› Evolution of dipolarization front events in a 6D global hybrid-Vlasov simulation - Lauri Pänkäläinen, Helsingin yliopisto = Helsingfors universitet = University of Helsinki
18:55-20:30 (1h35)
› Energetic particle experiment for the Plasma Observatory: geometric factor scaling based on THEMIS fluxes - Vassilis Angelopoulos, Dept. of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA
18:55-20:30 (1h35)
› Hybrid-kinetic modelling of the interaction between a planetary magnetosphere and a turbulent solar wind - Francesco Pucci, Istituto per la Scienza e Tecnologia dei Plasmi, Consiglio Nazionale delle Ricerche (ISTP-CNR)
18:55-20:30 (1h35)
› Bridging simulations and observations with machine learning: identification of reconnecting structures at collisionless shock waves - Imogen Gingell, University of Southampton
18:55-20:30 (1h35)
› Hyper Boris integrators for particle-in-cell (PIC) simulation - Seiji Zenitani, Space Research Institute, Austrian Academy of Sciences
18:55-20:30 (1h35)
› Plasma Observatory's Group on simulation NumerIcal support (GIANNI) - Markku Alho, Helsingin yliopisto = Helsingfors universitet = University of Helsinki
18:55-20:30 (1h35)
› Quasi thermal noise spectroscopy in a magnetospheric environment - Pietro Dazzi, Centre for Mathematical Plasma-Astrophysics [Leuven]
18:55-20:30 (1h35)
› Bi-Directional Energy Transfer Driven by Magnetic Reconnection - Raffaele Marino, CNRS - École Centrale de Lyon
18:55-20:30 (1h35)
› ESA F3 Mission Candidate: Magnetotail Dynamics Explorer - Andrew Fazakerley, Mullard Space Science Laboratory
18:55-20:30 (1h35)
› Comparison of noise levels of two different magnetometer types and space environments - Gerlinde Timmermann, Technische Universität Braunschweig = Technical University of Braunschweig [Braunschweig]
18:55-20:30 (1h35)
› Verification of Momentum Conservation in MMS Observations: A Step Toward Data-Driven Equation Discovery - Felipe Nathan deOliveira-Lopes, Max-Planck-Institut für Plasmaphysik [Garching]
18:55-20:30 (1h35)
› The Nature of Turbulence at Sub-Electron Scales in the Solar Wind - Shiladittya Mondal, Queen Mary University of London - Christopher Chen, Queen Mary University of London
18:55-20:30 (1h35)
› Progress of China Cross-scale Magnetospheric Explorer Mission - Yong Cun Zhang, NSSC, CAS
18:55-20:30 (1h35)
› Flat-top electron velocity distributions driven by nonlinear electrostatic waves - Sofia Zanelli, Università della Calabria [Arcavacata di Rende, Italia] = University of Calabria [Italy] = Université de Calabre [Italie]
18:55-20:30 (1h35)
› ECsim: Fully Kinetic Semi-Implicit Energy Conserving code for Magnetospheric Simulations - Harikrishnan Aravindakshan, Institut für Theoretische Physik, Ruhr University Bochum = Ruhr-Universität Bochum, Bochum
18:55-20:30 (1h35)
› Multi-spacecraft observations of energetic particles and their variability at strong IP shocks - Domenico Trotta, ESA
18:55-20:30 (1h35)
› J-Filtering: Unveiling Current Structures in Space Plasmas with Multipoint Data Analysis - Mehul CHAKRABORTY, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace
18:55-20:30 (1h35)
› Phase-Space Dynamics of Electron Acoustic Turbulence in 2D-2V Inhomogeneous Plasmas - Gabriele Celebre, Università della Calabria [Arcavacata di Rende, Italia] = University of Calabria [Italy] = Université de Calabre [Italie]
18:55-20:30 (1h35)
› SciQLop & Speasy: An Integrated Ecosystem for Modern Space Physics Data Analysis - Alexis Jeandet, Laboratoire de Physique des Plasmas
18:55-20:30 (1h35)
› Landau-Fluid Closures for Plasma Turbulence: Applications to Global Magnetospheric Modeling - Simon Lautenbach, Institute for Theoretical Physics I, Ruhr-University Bochum, Universitätsstraße 150, 44801 Bochum
18:55-20:30 (1h35)
› The "Plasma Astrophysics" working group for Plasma Observatory: an attempt to bridge heliospheric plasmas and far astrophysical systems - Oreste Pezzi, Istituto per la Scienza e Tecnologia dei Plasmi, Consiglio Nazionale delle Ricerche
18:55-20:30 (1h35)
› On the ripples propagating along the bow shock surface under quasi-perpendicular interaction with high-speed streams - Emanuele Cazzola, Laboratoire de Physique des Plasmas
18:55-20:30 (1h35)
› Plasma Observatory's Multi-Point and Advanced Data Analysis Methods Working Group - Giulia Cozzani, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, LPC2E, CNRS/CNES/University of Orléans
18:55-20:30 (1h35)
› Analysis of the Third-Order Law in MHD Turbulence with Distinct Dissipation Mechanisms - Fortugno Elisa Maria, Università degli Studi di Trento = University of Trento, Dipartimento di Fisica, Università della Calabria, 87036 Rende
18:55-20:30 (1h35)
› Large scale constraints on magnetic reconnection at the magnetopause from in situ observations - nicolas aunai, Laboratoire de Physique des Plasmas
18:55-20:30 (1h35)
› Dual Active Area Design for Plasma Observatory's Energetic Particle Experiment (EPE) - Ethan Tsai, Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USA
18:55-20:30 (1h35)
› The Lorentz Electron and Ion Analyzer - An instrument prototype based on EPE-M - Svea Jürgensen, Christian-Albrechts-Universität zu Kiel = Christian-Albrechts University of Kiel = Université Christian-Albrechts de Kiel
18:55-20:30 (1h35)
› Ion Energization and Acceleration Associated with Foreshock Bubbles: Results from a Hybrid-Vlasov Simulation and MMS Observations - Souhail Dahani, Department of Physics, University of Helsinki
18:55-20:30 (1h35)
PMO science: How are particles energized in near-Earth space plasmas ?
Auditorium
J. Stawarz
› Shock acceleration of nonthermal electrons in the heliosphere and beyond - Takanobu Amano, The University of Tokyo (INVITED ONLINE)
09:00-09:30 (30min)
› Electron energization by whistler waves in the Earth's magnetosheath - Ida Svenningsson, Department of Physics, Chalmers University of Technology, Gothenburg (INVITED)
09:30-09:50 (20min)
› Evidence for self-organization between multiscale plasma structures and energy dissipation via gradient tensor geometric invariants - Simone Benella, Istituto di Astrofisica e Planetologia Spaziali - INAF
09:50-10:05 (15min)
› Universality of Markovian Turbulence in Earth's Magnetosphere Based on MMS Data. - Dariusz Wójcik, Space Research Centre, Polish Academy of Sciences, Solar System Physics and Astrophysics Division (INVITED)
10:05-10:25 (20min)
PMO science: How are particles energized in near-Earth space plasmas ?
Auditorium
M. E. Innocenti
› Electron Energy Partition during Magnetic Reconnection - Seiji Zenitani, Space Research Institute, Austria (INVITED)
10:55-11:25 (30min)
› Exploring particle energization in turbulent plasma using multi-point observations - Alexandros Chasapis, LASP, Boulder (ONLINE)
11:25-11:40 (15min)
› Universal Scaling Law for Particle Energization in Plasmas - Mitsuo Oka, UC Berkeley (INVITED)
11:40-12:00 (20min)
› Energy conversion and partitioning associated with magnetic reconnection - Benoit Lavraud, Laboratoire d'Astrophysique de Bordeaux (INVITED)
12:00-12:20 (20min)
PMO science: How are particles energized in near-Earth space plasmas ?
Auditorium
C. Norgen
› Magnetic reconnection at collisionless shocks: current understanding and future investigations - Konrad Steinvall, Department of Physics, Chalmers University of Technology, Gothenburg (INVITED ONLINE)
13:20-13:50 (30min)
› Non-Maxwellianity of Ion Velocity Distributions in the Earth's Magnetosheath - Louis Richard, Swedish Institute of Space Physics
13:50-14:05 (15min)
› Particle Heating, Plasma Turbulence, and the Need for Multipoint Measurements - Davide Manzini, Queen Mary University of London (INVITED)
14:05-14:25 (20min)
PMO science: Which processes dominate energy transport and drive coupling between different regions of magnetospheric system ?
Auditorium
F. Valentini
› Which are the key plasma instabilities involved in energy transport - Jonathan Rae, Northumbria University (INVITED)
14:25-14:55 (30min)
› Magnetotail plasma eruptions driven by magnetic reconnection and kinetic instabilities, and a bit further - Markku Alho, University of Helsinki (INVITED)
14:55-15:15 (20min)
PMO science: Which processes dominate energy transport and drive coupling between different regions of magnetospheric system ?
Auditorium
Y. Khotyaintsev
› Interplay of Magnetic Reconnection and Current Sheet Kink Instability in the Earth's Magnetotail - Giulia Cozzani, LPC2E, CNRS/CNES/University of Orléans (INVITED)
15:45-16:05 (20min)
› How would PMO capture Kelvin-Helmholtz Instability? - Adriana Settino, Space Research Institute (IWF), OEAW, Graz (INVITED)
16:05-16:25 (20min)
› How do plasma jets interact with Earth's dipole field? - Evgeny Panov, Space Research Institute, Austrian Academy of Sciences (INVITED)
16:25-16:55 (30min)
› H+ and O+ velocity distributions in a dipolarization flux bundle observed by Cluster on 7 October, 2002 - Timo Pitkänen, Institute of Space Sciences, School of Space Science and Technology, Shandong University, Weihai
16:55-17:10 (15min)
› Global modeling of the mesoscale buildup of the ring current and its role in magnetosphere-ionosphere coupling - Kareem Sorathia, Johns Hopkins University Applied Physics Laboratory (INVITED ONLINE)
17:10-17:30 (20min)
› Wave-particle interactions in the magnetosphere up to the outer boundary - Ondřej Santolík, Institute of Atmospheric Physics of the Czech Academy of Sciences (INVITED)
17:30-17:50 (20min)
PMO science: Which processes dominate energy transport and drive coupling between different regions of magnetospheric system ?
Auditorium
M. F. Marcucci
› How do FACs connect different regions of the Magnetospheric System ? - Colin Forsyth, Mullard Space Science Laboratory (INVITED)
09:00-09:30 (30min)
› Field Aligned Currents driven by Bursty Bulk Flows - Vanina Lanabere, Swedish Institute of Space Physics, Uppsala (INVITED)
09:30-09:50 (20min)
› A new approach to quantifying data-model comparisons at mesoscales - Sara Gasparini, Univ. of Bergen, Norway (INVITED)
09:50-10:10 (20min)
› Coupling of Bursty Bulk Flows to the Ionosphere-Thermosphere as Observed by Cluster-Swarm Conjugate Events and Prospects for Plasma Observatory - Octav Marghitu, Institute of Space Science [Bucharest-Măgurele]
10:10-10:25 (15min)
› A different type of plasma emissions below the electron cyclotron frequency in the upper atmosphere - Hanna Rothkaehl, Space Research Centre PAS
10:25-10:45 (20min)
PMO science: Which processes dominate energy transport and drive coupling between different regions of magnetospheric system ?
Auditorium
M. Alho
› Energy partitioning in the aftermath of tail reconnection - Vassilis Angelopoulos, Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USA (INVITED)
11:15-11:45 (30min)
› Anisotropy of Yaglom's law -- a multipoint multiscale analysis using PO, HS and MMS - Francesco Pecora, University of Delaware [Newark]
11:45-12:00 (15min)
› 2D fully kinetic PIC simulations of dayside magnetic reconnection in the presence of cold ions and a moderate guide field. - Mohammed Baraka, Laboratoire de Physique des Plasmas (INVITED)
12:00-12:20 (20min)
› Ground-based observations of the magnetosphere: current and future capabilities - Maxime Grandin, Finnish Meteorological Institute (INVITED ONLINE)
13:20-13:40 (20min)
› Particle energization in astrophysical shocks - open questions and links to helioshperic shock physics - Jacek Niemiec, Institute of Nuclear Physics, Polish Academy of Sciences (INVITED)
13:40-14:00 (20min)
› Kinetic Properties of the Reconnection Electron Diffusion Region, Explored Through Theory and Experiment - Jan Egedal, Department of Physics, University of Wisconsin-Madison (INVITED)
14:00-14:20 (20min)
› Machine learning identification of magnetopause boundary layer signatures to constrain the location of the global reconnection line. - Ambre Ghisalberti, Laboratoire de Physique des Plasmas
14:20-14:35 (15min)
› Bridging in Situ Satellite Measurements and Simulations Using Machine Learning: Applications to Magnetic Reconnection and Turbulence - Cara Waters, Queen Mary, University of London, Imperial College London
14:35-14:50 (15min)
› Machine Learning for Enhanced Plasma Observations: From Cluster to the Plasma Observatory - George Miloshevich, KULeuven (INVITED)
14:50-15:10 (20min)
Loading... 
Auditorium
