Investigating the Dynamics of Planetary Magnetotails


An ISSI international team

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Welcome

Introduction

We are an international team of 13 scientists funded by the International Space Science Institute and engaged in a project to study the dynamics of planetary magnetotails.

Please feel free to explore our site and read our proposal and contact the team coordinators Caitriona Jackman, Chris Arridge, Nicolas André, or the site webmaster.



Abstract

Spacecraft observations have established that all magnetised planets interact strongly with the solar wind and possess well-developed magnetic tails. We wish to study reconnection, convection, and charged particle acceleration in the magnetic tails of Mercury, Earth, Jupiter and Saturn. These fundamental physical processes are common to all these planetary environments and relate to a complex chain of events that ultimately release mass and energy in magnetised configurations. The great differences in solar wind conditions, planetary rotation rates, ionospheric conductivity, and physical dimensions from Mercury’s small magnetosphere to the giant magnetospheres of Jupiter and Saturn, provide an outstanding opportunity to extend our understanding of the influence of these factors on these basic processes. We will draw together data analysis experts and global modellers to build up a full picture of small- and large-scale dynamics. We will make use of numerous data sets from MESSENGER, Geotail, Cluster, THEMIS, Galileo, New Horizons, Cassini, and the Hubble Space Telescope (HST) to name but a few, together with sophisticated simulation and modelling tools in order to probe in-situ and remotely the deep magnetotails of these planets.



Team

Team photo
Team LeaderCaitriona Jackman
Deputy Team LeaderChris Arridge
Deputy Team LeaderNicolas André


Core Team

Team member

Institution

Country

Expertise

Caitriona Jackman ICL UK Cassini MAG
Chris Arridge MSSL/UCL UK Cassini MAG/CAPS
Nicolas Andre CESR France Cassini MAPS
Fran Bagenal LASP, U. Colorado USA Voyager PLS, Galileo IDS, Deep Space 1, New Horizons, Juno
Joachim Birn LANL USA Global MHD Modelling
William Farrell NASA/GSFC USA Voyager, Cassini RPWS, WIND, DSX
Mervyn Freeman BAS UK SuperDARN, Substorm models
Xianzhe Jia U. Michigan USA Cassini IDS, Global MHD Modelling
Steve Milan U. Leicester UK SuperDARN, CUTLASS, KuaFu-B, Bepi-Columbo
Aikaterini Radioti U. Liege Belgium HST, Cassini UVIS, Galileo EPD
James Slavin NASA/GSFC USA MESSENGER, MMS, Bepi-Columbo, Cluster, WIND
Martin Volwerk

OEAWAustriaGalileo MAG/Cluster FGM/THEMIS FGM

ICL: Imperial College London, MSSL/UCL: Mullard Space Science Laboratory, University College London, CESR: Centre d’Etude Spatiale des Rayonnements, LASP/U. Boulder : Laboratory for Atmospheric and Space Physics, University of Colorado, IDS: Inter-disciplinary scientist, LANL: Los Alamos National Research Laboratory, NASA/GSFC: Goddard Space Flight Centre, BAS: British Antarctic Survey, U. Michigan: University of Michigan, U. Leicester: University of Leicester, U. Liege: University of Liege, OEAW: Osterreichische Akademie der Wissenschaften, U.Washington: University of Washington, UCLA: University of California Los Angeles.



Young Scientists

Team member

Institution

Country

Expertise

Ariah Kidder U. Washington USA Global numerical simulations
Marissa Vogt UCLA USA Galileo MAG
Andrew Walsh MSSL/UCL UK Cluster PEACE, CIS, FGM, IMAGE



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Please contact the webmaster with any questions/corrections.