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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 27, issue 5 | Copyright

Special issue: Ninth International Conference on Substorms (ICS9)

Ann. Geophys., 27, 2191-2204, 2009
https://doi.org/10.5194/angeo-27-2191-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.

  13 May 2009

13 May 2009


In-situ observation of ULF wave activities associated with substorm expansion phase onset and current disruption

J. Liang1,2, W. W. Liu1, E. F. Donovan2, and E. Spanswick2 J. Liang et al.
  • 1Space Science Branch, Canadian Space Agency, St-Hubert, Quebec, Canada
  • 2Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada

Abstract. In this paper we present two substorm events with coordinated ground-based and in-situ THEMIS observations, and focus our interest on the wave activities in Pi1 and Pi2 bands from minutes before the substorm expansion phase (EP) onset to minutes after the local current disruption (CD). We find that Pi2 band (40–100 s) wave appears 1–2 min before the substorm onset and last over the entire EP interval, while higher-frequency wave within Pi1 band (10–30 s) emerges within few tens of seconds after the EP onset, intensifies during the local CD, and fades afterwards. The pre-onset Pi2 waves are attributed to a ballooning mode which acts as the seed perturbation to the substorm EP onset process. The azimuthal wavenumber estimated from the Doppler shift nature of the ballooning mode is consistent with the longitudinal "wavelength" inferred from the onset auroral structures. The Pi1 waves appearing within few tens of seconds after the EP onset are interpreted as supportive of a two-fluid instability mode of thin current sheet investigated in an accompanying paper (Liu and Liang, 2009). During the local CD, broadband wave activities from Pi2 band to well above the ion gyrofrequency are observed, suggesting the coexistence of various plasma instabilities featuring different frequency ranges.

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