FastFind »   Lastname: doi:10.1029/ Year: Advanced Search  

AGU: Geophysical Research Letters

 

Keywords

  • substorm
  • aurora
  • onset

Index Terms

  • Magnetospheric Physics: Substorms
  • Magnetospheric Physics: Auroral phenomena
  • Magnetospheric Physics: Magnetosphere/ionosphere interactions
  • Magnetospheric Physics: Magnetospheric configuration and dynamics

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 36, L24104, 6 PP., 2009
doi:10.1029/2009GL041476

Equatorward moving auroral signatures of a flow burst observed prior to auroral onset

L. Kepko

Space Science Center, University of New Hampshire, Durham, New Hampshire, USA

E. Spanswick

Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada

V. Angelopoulos

Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California, USA

E. Donovan

Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada

J. McFadden

Space Sciences Laboratory, University of California at Berkeley, California, USA

K.-H. Glassmeier

Institute of Geophysics and Extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, Germany

J. Raeder

Space Science Center, University of New Hampshire, Durham, New Hampshire, USA

H. J. Singer

Space Weather Prediction Center, NOAA, Boulder, Colorado, USA

We present observations of a substorm that occurred on February 25, 2008. Auroral onset was observed with a multi-spectral (λ = 427.8, 557.7 and 630.0 nm) and white light all sky imager at Gillam, Canada. An equatorward moving diffuse auroral patch was observed in the λ = 630.0 nm images at least six minutes prior to auroral onset. This form emerged from the background noise poleward of the eventual onset arc and intensified as it moved equatorward. Auroral expansion onset occurred when this form reached the onset arc location. Flows were detected by THEMIS probes P3 (TH-D) and P4 (TH-E) near X ∼ −11 RE nearly 90 seconds prior to auroral expansion. A small discrete arc was observed in the λ = 557.7 nm images at the westward and equatorward edge of the diffuse 630.0 nm patch nearly 2 minutes prior to expansion onset, suggesting a field-aligned current of a substorm current wedge geometry. We conclude that the equatorward moving λ = 630.0 nm diffuse auroral patch was generated by processes associated with an earthward moving flow burst that formed prior to auroral substorm onset.

Received 23 October 2009; accepted 30 November 2009; published 31 December 2009.

Citation: Kepko, L., E. Spanswick, V. Angelopoulos, E. Donovan, J. McFadden, K.-H. Glassmeier, J. Raeder, and H. J. Singer (2009), Equatorward moving auroral signatures of a flow burst observed prior to auroral onset, Geophys. Res. Lett., 36, L24104, doi:10.1029/2009GL041476.

Cited By

Please wait one moment ...