Joint Cluster-Plasma Observatory workshop

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)