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8:00 - 9:00 (1h)
Registration
Registration
9:00 - 9:10 (10min)
Welcome & Logistics
Welcome & Logistics
9:10 - 10:45 (1h35)
Cluster mission legacy
Auditorium
P. Canu
› 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)
10:45 - 11:25 (40min)
Coffee break
Hall
11:25 - 12:45 (1h20)
Cluster mission legacy
Auditorium
O. Le Contel
› 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)
12:45 - 13:45 (1h)
Lunch
Self Cocagne
13:45 - 15:25 (1h40)
Cluster mission legacy
Auditorium
P. Escoubet
› 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)
15:25 - 16:05 (40min)
Coffee break
Hall
16:05 - 18:15 (2h10)
Cluster mission legacy
Auditorium
M. Taylor
› 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)
18:15 - 19:45 (1h30)
Posters Session I
Hall
A. Vaivads
› 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)
19:45 - 21:00 (1h15)
Icebreaker Cocktail @ FIAP Conference Center
Hall
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9:00 - 10:20 (1h20)
Plasma Observatory mission
Auditorium
M. F. Marcucci
› ESA Welcome & M7 Status Update
- Yannis Zouganelis, Agence Spatiale Européenne (INVITED ONLINE)
09:00-09:15 (15min)
› French Contribution to Plasma Observatory Mission
- Cécile Fiachetti, Centre National d'Études Spatiales (INVITED)
09:15-09:30 (15min)
› Plasma Observatory: mission overview
- M. Federica Marcucci (IAPS-INAF) & Alessandro Retino (LPP-CNRS)
09:30-10:00 (30min)
› Plasma Observatory Mission: ESA Phase A scientific organization
- Matt Taylor, ESA - ESTEC (Netherlands)
10:00-10:20 (20min)
10:20 - 11:00 (40min)
Coffee break
Hall
11:00 - 12:40 (1h40)
Plasma Observatory mission
Auditorium
A. Retino
› Plasma Observatory Mission Introduction - from the ESA perspective
- Uwe Derz, European Space Agency (INVITED)
11:00-11:30 (30min)
› Constellation design and optimisation for the Plasma Observatory mission
- Théo James, ESA - ESTEC (Netherlands) (INVITED)
11:30-11:50 (20min)
› Plasma Observatory Payload Overview - from the ESA perspective
- Anamarija Stankov, European Space Agency (INVITED)
11:50-11:20 (-1h-30)
› Science Operations for Plasma Observatory
- Andrew Walsh, European Space Agency (INVITED)
12:20-12:40 (20min)
12:40 - 13:40 (1h)
Lunch
Self Cocagne
13:40 - 15:00 (1h20)
Plasma Observatory mission
Auditorium
G. Henaff
› 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)
15:00 - 15:40 (40min)
Coffee break
Hall
15:40 - 17:40 (2h)
Plasma Observatory mission
Auditorium
M. Michelagnoli
› 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)
17:40 - 19:00 (1h20)
Free time
19:00 - 22:00 (3h)
Cluster Documentary @ Majestic movie theater in Passy
Introduction by authors, welcome cocktail and projection
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9:00 - 10:30 (1h30)
Science & technical splinters
Splinters agenda separately sent by email
10:30 - 11:00 (30min)
Coffee break
Hall
11:00 - 12:30 (1h30)
Science & technical splinters
Splinters agenda separately sent by email
12:30 - 13:30 (1h)
Lunch
Self Cocagne
13:30 - 15:30 (2h)
Science & technical splinters
Splinters agenda separately sent by email
15:30 - 16:00 (30min)
Coffee break
Hall
16:00 - 18:55 (2h55)
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)
18:55 - 20:30 (1h35)
Posters Session II
Hall
H. Hietala
› 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)
20:30 - 22:30 (2h)
Social dinner @ FIAP Conference Center
Hall
|
9:00 - 10:25 (1h25)
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)
10:25 - 10:55 (30min)
Coffee break
Hall
10:55 - 12:20 (1h25)
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)
12:20 - 13:20 (1h)
Lunch
Self Cocagne
13:20 - 14:25 (1h05)
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)
14:25 - 15:15 (50min)
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)
15:15 - 15:45 (30min)
Coffee break
Hall
15:45 - 17:50 (2h05)
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)
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9:00 - 10:45 (1h45)
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)
10:45 - 11:15 (30min)
Coffee break
Hall
11:15 - 12:20 (1h05)
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)
12:20 - 13:20 (1h)
Lunch
Self Cocagne
13:20 - 15:10 (1h50)
Plasma Observatory broader impact
Auditorium
L. Griton
› 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)
15:10 - 15:40 (30min)
Coffee break
Hall
15:40 - 17:00 (1h20)
Yellow Book common open discussion and concluding remarks
Auditorium
M. F. Marcucci, A. Retino & M. Taylor
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