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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 28, issue 10 | Copyright
Ann. Geophys., 28, 1847-1857, 2010
https://doi.org/10.5194/angeo-28-1847-2010
© Author(s) 2010. This work is distributed under
the Creative Commons Attribution 3.0 License.

  06 Oct 2010

06 Oct 2010

Lower-thermospheric wind fluctuations measured with an FPI during pulsating aurora at Tromsø, Norway

S. Oyama1,2, K. Shiokawa1, J. Kurihara1,*, T. T. Tsuda1, S. Nozawa1, Y. Ogawa3, Y. Otsuka1, and B. J. Watkins2 S. Oyama et al.
  • 1Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan
  • 2Geophysical Institute, University of Alaska Fairbanks, Fairbanks, AK, USA
  • 3National Institute of Polar Research, Tokyo, Japan
  • *now at: Graduate School of Science, Hokkaido University, Sapporo, Japan

Abstract. Simultaneous observations were conducted with a Fabry-Perot Interferometer (FPI) at a wavelength of 557.7 nm, an all-sky camera at a wavelength of 557.7 nm, and the European Incoherent Scatter (EISCAT) UHF radar during the Dynamics and Energetics of the Lower Thermosphere in Aurora 2 (DELTA-2) campaign in January 2009. This paper concentrated on two events during periods of pulsating aurora. The lower-thermospheric wind velocity measured with the FPI showed obvious fluctuations in both vertical and horizontal components. Of particular interest is that the location of the fluctuations was found in a darker area that appeared within the pulsating aurora. During the same time period, the EISCAT radar observed sporadic enhancements in the F-region backscatter echo power, which suggests the presence of low-energy electron (1 keV or lower) precipitation coinciding with increase in amplitude of the electromagnetic wave (at the order of 10 Hz or higher). While we have not yet identified the dominant mechanism causing the fluctuations in FPI-derived wind velocity during the pulsating aurora, the frictional heating energy dissipated by the electric-field perturbations may be responsible for the increase in ionospheric thermal energy thus modifying the local wind dynamics in the lower thermosphere.

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