Are small-scale field-aligned currents and magnetosheath-like particle precipitation signatures of the same low-altitude cusp?

Details Are small-scale field-aligned currents and magnetosheath-like particle precipitation signatures of the same low-altitude cusp? Are small-scale field-aligned currents and magnetosheath-like particle precipitation signatures of the same low-altitude cusp?

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009adspr..43...41w&link_type=abstract

Advances in Space Research, Volume 43, Issue 1, p. 41-46.

Physics

1

Scientific paper

We examined some 75 observations from the low-altitude Earth orbiting DMSP, Ørsted and CHAMP satellites which were taken in the region of the nominal cusp. Our objective was to determine whether the actually observed cusp locations as inferred from magnetosheath-like particle precipitation (“particle cusp”) and intense small-scale magnetic field variations (“current cusp”), respectively, were identical and were consistent with the statistically expected latitude of the cusp derived from a huge number of charged particle spectrograms (“statistical cusp”). The geocentric coordinates of the satellites were converted into AACGM coordinates, and the geomagnetic latitude of the cusp boundaries (as indicated by precipitating particles and small-scale field-aligned currents) set in relation to the IMF-Bz dependent latitude of the equatorward boundary of the statistical cusp. We find that the actually observed latitude of the particle cusp matches well the statistically expected latitude while the current cusp appears to cover most of the statistical cusp and also a ≈1° wide section beyond the equatorward boundary of the statistical cusp. This leads us to suggest that intense small-scale field-aligned currents are generated in the cusp but also in the transition zone between the low-latitude boundary layer (LLBL) and the cusp, probably within both regimes, the cusp and the open LLBL. The small-scale field-aligned currents are possibly a consequence of turbulence and/or instabilities associated with the process of opening previously closed magnetospheric field lines and merging them with the interplanetary magnetic field.

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