Entry of the POLAR spacecraft into the polar cusp under northward IMF conditions

• Published in: Geophysical research letters 1998-08, Vol.25 (15), p.3015-3018
• Main Authors: Russell, C. T., Fedder, J. A., Slinker, S. P., Zhou, X.-W., Le, G., Luhmann, J. G., Fenrich, F. R., Chandler, M. O., Moore, T. E., Fuselier, S. A.
• Format: Article
• Language: English
• Subjects: Earth, ocean, space; Exact sciences and technology; External geophysics; Interaction between magnetosphere and interplanetary space; Physics of the magnetosphere
• ISSN: 0094-8276; 1944-8007
• DOI: 10.1029/98GL00355

On May 29, 1996 from 0200 to 0800 UT the solar wind dynamic pressure was high ranging from 6 to 8 nPa and the interplanetary field was almost due northward, ranging from 10 to 15 nT in BZ GSM. Even at apogee the POLAR spacecraft should not have entered the magnetosheath according to recent scaling laws. However, the magnetic field was greatly depressed below the value expected indicating the presence of significant plasma energy density throughout the high latitude magnetosphere surrounding the cusp. The presence of this plasma is confirmed by the plasma instrumentation on board the spacecraft. While the entry into this nearly stagnant plasma was gradual, the exit on to polar cap field lines was abrupt. We interpret these observations in terms of the post‐cusp reconnection of the strongly northward interplanetary magnetic field.