An extended study of the low‐latitude boundary layer on the dawn and dusk flanks of the magnetosphere

Authors:
  • DMD. G. Mitchell
    D. G. Mitchell
  • FKF. Kutchko
    F. Kutchko
  • DWD. J. Williams
    D. J. Williams
  • TET. E. Eastman
    T. E. Eastman
  • LFL. A. Frank
    L. A. Frank
Publisher website
Google Scholar
Abstract
We present a study of the low‐latitude boundary layer (LLBL) using ISEE 1 energetic particle, plasma, and magnetic field data obtained during numerous traversals of the LLBL that occurred on 66 ISEE 1 passes through the magnetospheric flank LLBL region. We use energetic particle distributions to determine dawn and dusk LLBL behavior and topology for varying orientations of the magnetosheath and/or interplanetary magnetic field (M/IMF), for different local times, and for changing levels of geomagnetic activity (Kp). This study corroborates and extends the earlier work of Williams et al. (1985) who presented a detailed study of two (dusk and dawn) ISEE 1 passes through the LLBL region for the case of northward M/IMF. We find that the dawn and dusk LLBL are on closed geomagnetic field lines for northward M/IMF but are on a combination of closed and open field lines for a southward M/IMF. The energetic particle distributions show that cases of reverse‐draped field lines in the LLBL are consistent with an open field line topology. In addition, we find that the LLBL is thicker (thinner) for northward (southward) M/IMF and becomes thicker with increasing distance from the subsolar point. LLBL electric fields nominally are in the few (3–5) millivolts per meter range and display an apparent maximum value of ∼10 mV/m. These electric fields capture magnetospherically drifting particles as they approach the LLBL and propel them tailward. In this way, the plasma sheet is the dominant source of energetic (≳10 keV) particles in the LLBL while the magnetosheath appears to be the dominant source for lower‐energy (≲10 keV) LLBL particles.

This publication has 18 references indexed in Scilit: