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)
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Auditorium
