Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter
1Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK
2Lockheed Martin ATC, Palo Alto, USA
3The Aerospace Corporation, Los Angeles, CA, USA
Correspondence to: L. J. Baddeley
Abstract. HF radar backscatter, which has been artificially-induced by a high power RF facility such as the EISCAT heater at Tromsø, has provided coherent radar ionospheric electric field data of unprecedented temporal resolution and accuracy. Here such data are used to investigate ULF wave processes observed by both the CUTLASS HF radars and the EISCAT UHF radar. Data from the SP-UK-OUCH experiment have revealed small-scale (high azimuthal wave number, m <approx> -45) waves, predominantly in the morning sector, thought to be brought about by the drift-bounce resonance processes. Conjugate observations from the Polar CAM-MICE instrument indicate the presence of a non-Maxwellian ion distribution function. Further statistical analysis has been undertaken, using the Polar TIMAS instrument, to reveal the prevalence and magnitude of the non-Maxwellian energetic particle populations thought to be responsible for generating these wave types.
Key words. Ionosphere (active experiments; wave-particle interactions) Magnetospheric physics (MHD waves and instabilities)
Baddeley, L. J., Yeoman, T. K., Wright, D. M., Davies, J. A., Trattner, K. J., and Roeder, J. L.: Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter, Ann. Geophys., 20, 1487-1498, doi:10.5194/angeo-20-1487-2002, 2002.