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)
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