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)
Loading... 
Auditorium
