A Statistical Analysis of Spatial and Temporal Phase Evolution in Intermediate-m Ultra-low Frequency (ULF) Wave Observations Using the Hankasalmi SuperDARN Radar and Magnetometer Data
Abstract
The characterisation of a ULF wave event over a 3-hour interval (0000-0300 UT) on 13th May, 2016, studied with the Hankasalmi SuperDARN radar and the IMAGE magnetometer array suggests an equatorward latitudinal and eastward longitudinal phase propagation with an effective azimuthal wave number, m of 13.1 ± 1. The wave has been interpreted as resulting from drifting electrons of energies of 35 ± 5 KeV in a drift resonance condition linked to particle populations from a substorm onset at about 1 hour prior to the wave occurrence. The phase characteristics of this wave seem to evolve at 0200 UT when a distinct Pc4 wave was also observed in the magnetometer data with a poleward latitudinal and a westward longitudinal phase propagation (m of -29.5 ± 1). The Pc4 wave is associated with a second harmonic mode driven by a drift-bounce resonance interaction with proton energies of 10 ± 3 KeV from a separate substorm occurrence. We present a statistical analysis of 18 similar ULF wave events also linked to substorm-injected particle populations using the Hankasalmi SuperDARN radar and IMAGE magnetometer array data.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2019
- Bibcode:
- 2019AGUFMSM23F3285M
- Keywords:
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- 2483 Wave/particle interactions;
- IONOSPHERE;
- 2752 MHD waves and instabilities;
- MAGNETOSPHERIC PHYSICS;
- 2772 Plasma waves and instabilities;
- MAGNETOSPHERIC PHYSICS;
- 2784 Solar wind/magnetosphere interactions;
- MAGNETOSPHERIC PHYSICS