Annales Geophysicae (Oct 2006)

Evidence of standing waves during a Pi2 pulsation event observed on Cluster

  • A. B. Collier,
  • A. B. Collier,
  • A. R. W. Hughes,
  • L. G. Blomberg,
  • P. R. Sutcliffe

DOI
https://doi.org/10.5194/angeo-24-2719-2006
Journal volume & issue
Vol. 24
pp. 2719 – 2733

Abstract

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Observations of Pi2 pulsations at middle and low latitudes have been explained in terms of cavity mode resonances, whereas transients associated with field-aligned currents appear to be responsible for the high latitude Pi2 signature. Data from Cluster are used to study a Pi2 event observed at 18:09 UTC on 21 January 2003, when three of the satellites were within the plasmasphere (L=4.7, 4.5 and 4.6) while the fourth was on the plasmapause or in the plasmatrough (L=6.6). Simultaneous pulsations at ground observatories and the injection of particles at geosynchronous orbit corroborate the occurrence of a substorm. Evidence of a cavity mode resonance is established by considering the phase relationship between the orthogonal electric and magnetic field components associated with radial and field-aligned standing waves. The relative phase between satellites located on either side of the geomagnetic equator indicates that the field-aligned oscillation is an odd harmonic. Finite azimuthal Poynting flux suggests that the cavity is effectively open ended and the azimuthal wave number is estimated as m~13.5.