SM52B:
Synergistic Studies of Global and Kinetic Magnetospheric Processes using Multipoint Space and Ground Assets II


Session ID#: 11112

Session Description:
Considering all in-situ assets in combination with distributed ground based arrays, we have a robust Heliophysics system observatory for probing our complex space environment. This is in fact what is needed for exploring global connections and their interplay with meso-scale and kinetic processes, signatures of which can be seen in various regions: from the bow shock, magnetopause, dayside cusp, nightside plasma sheet to the inner magnetopshere, aurora and polar cap. It is necessary to understand how turbulence transports energy from large scales to small scales, how reconnection converts magnetic energy to plasma energy, how small-scale processes control large-scale phenomena, and how thin boundary layers are formed and sustained in the presence of plasma turbulence. We solicit a broad range of presentations using existing and future assets, including satellites (such as THEMIS, Van Allen Probes, Cluster, Geotail and MMS), rockets, balloons and ground-based networks such as optical, radio and magnetometer arrays.
Primary Convener:  Marilia Samara, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Conveners:  C Philippe Escoubet, ESTEC, Noordwijk, 2201, Netherlands, Toshi Nishimura, University of California Los Angeles, Los Angeles, CA, United States and Arnaud Masson, European Space Agency, ESAC, SCI-SAA, Madrid, Spain
Chairs:  Marilia Samara, NASA Goddard Space Flight Center, Greenbelt, MD, United States and C Philippe Escoubet, ESTEC, Noordwijk, 2201, Netherlands
OSPA Liaison:  Toshi Nishimura, University of California Los Angeles, Los Angeles, CA, United States
Index Terms:

2704 Auroral phenomena [MAGNETOSPHERIC PHYSICS]
2736 Magnetosphere/ionosphere interactions [MAGNETOSPHERIC PHYSICS]
2740 Magnetospheric configuration and dynamics [MAGNETOSPHERIC PHYSICS]
2784 Solar wind/magnetosphere interactions [MAGNETOSPHERIC PHYSICS]

Abstracts Submitted to this Session:

Michael A Balikhin, Univ Sheffield, Sheffield, United Kingdom, Yuri Shprits, University of California Los Angeles, Los Angeles, United States and Simon N Walker, University of Sheffield, Sheffield, S10, United Kingdom
Sergio Toledo Redondo1,2, Mats Andre3, Andris Vaivads3, Yuri V Khotyaintsev3, Benoit Lavraud4, Andrey V Divin5, Nicolas Aunai6 and Daniel Bruce Graham3, (1)European Space Agency, SRE-ODS, Villanueva De La CaƱada, Spain, Spain, (2)IRAP, Toulouse, France, (3)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (4)Laboratoire d'astrophysique de Bordeaux, Pessac, France, (5)St. Petersburg State university, St Petersburg, Russia, (6)Laboratoire de Physique des Plasmas, CNRS, Paris, France
Vassilis Angelopoulos1, Heli Hietala2, Zixu Zixu Liu3, Stephen B Mende4, Tai Phan5, Toshi Nishimura6, Robert J Strangeway6, James L Burch7, Thomas Earle Moore8 and Barbara L Giles9, (1)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, United States, (2)Imperial College London, Department of Physics, London, United Kingdom, (3)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, (4)University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States, (5)University of California Berkeley, Berkeley, CA, United States, (6)University of California Los Angeles, Los Angeles, CA, United States, (7)Southwest Research Institute, San Antonio, TX, United States, (8)NASA Goddard Space Flight Ctr, Greenbelt, United States, (9)NASA Goddard Space Flight Center, Greenbelt, United States