<p>We examine a 6‐day traversal of the magnetotail by the ARTEMIS satellites during an interval of prolonged northward IMF. The electrostatic analyzer (ESA) onboard the ARTEMIS spacecraft measures high ion and electron fluxes at approximately 60 RE downtail in regions of the magnetotail which would normally be the magnetotail lobe, containing open flux evacuated of plasma. We interpret these observations as trapped plasma on closed magnetic flux indicating that the magnetotail is closed or partially closed but extends at least as far as ∼60 RE downtail. We find that the occurrence of plasma in the magnetotail and the closure of the magnetosphere results in distinct changes to the magnetotail structure including a reduction in the magnetic field strength and pressure as well as a narrowing of the tail by approximately 20 RE.</p>
Funding
A Consolidated Grant Proposal for Solar and Planetary Science at the University of Leicester, 2019 - 2022
We acknowledge NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS/ARTEMIS Mission. Specifically, C. W. Carlson and J. P. McFadden for use of ESA data (McFadden et al., 2008), K. H. Glassmeier, U. Auster and W. Baumjohann for the use of FGM data (Auster et al., 2008) provided under the lead of the Technical University of Braunschweig and with financial support through the German Ministry for Economy and Technology and the German Center for Aviation and Space (DLR) under contract 50 OC 0302. We also acknowledge the low resolution (5-min) OMNI data used in this study (King & Papitashvili, 2005) provided by the NASA Goddard Space Flight Center, Space Physics Data Facility and publicly available at https://omniweb.gsfc.nasa.gov/html/ow_data.html.