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Radar observations of ion cyclotron waves associated with two barium shaped-charge releases

Journal Article · · Journal of Geophysical Research; (United States)
; ;  [1];  [2]; ;  [3]
  1. Cornell Univ., Ithaca, NY (USA)
  2. Aerospace Corp., Los Angeles, CA (USA)
  3. System Planning Corp., Houston, TX (USA)

A 50-MHz Doppler radar interferometer and a 138-MHz Doppler radar were operated from Kennedy Space Center to study 3-m and 1-m plasma waves associated with two shaped-charged barium releases from Wallops Island, Virginia, on May 13, 1986. During the first release, interferometer and Doppler power spectral studies showed the existence of short-lived (<2 s) coherent 3-m and 1-m waves centered near 30 Hz. The 3-m waves were located about 100 km above the release on a magnetic field line in contact with the first release. No radar backscatter was observed by the radars during the second release. The coherent 30-Hz radar echoes associated with the first barium release are very similar to some natural occurring auroral radar echoes that are believed to be generated by resistive current-driven electrostatic ion cyclotron waves. A detailed linear dispersion analysis of electrostatic ion cyclotron (EIC) waves showed that only 3-m O{sup +} EIC waves were unstable for field-aligned electron drifts greater than 0.7{upsilon}{sub the} at the altitude of 510 km in a multispecies (O{sup +}, NO{sup +}, or similarly O{sub 2}{sup +}) ionospheric plasma. The authors interpret the 30-Hz waves seen by the two radars far above the release as strong electrostatic ion cyclotron waves generated by intense field-aligned currents associated with the barium stream acting like an MHD generator coupled to the ionospheres.

OSTI ID:
5378099
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 95:A12; ISSN JGREA; ISSN 0148-0227
Country of Publication:
United States
Language:
English