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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 14, issue 12
Ann. Geophys., 14, 1317–1327, 1996
https://doi.org/10.1007/s00585-996-1317-7
© European Geosciences Union 1996

Special issue: VIIIe EISCAT

Ann. Geophys., 14, 1317–1327, 1996
https://doi.org/10.1007/s00585-996-1317-7
© European Geosciences Union 1996

  31 Dec 1996

31 Dec 1996

PMSE observations at three different frequencies in northern Europe during summer 1994

J. Bremer1, P. Hoffmann1, A. H. Manson2, C. E. Meek2, R. Rüster3, and W. Singer1 J. Bremer et al.
  • 1Institut für Atmosphärenphysik, D-18225 Kühlungsborn, Germany
  • 2Institute of Space and Atmospheric Studies, University of Saskatchewan, Saskatoon, S7N 5E2, Canada
  • 3Max-Planck-Institut für Aeronomie, D-37189 Katlenburg-Lindau, Germany

Abstract. Simultaneous observations of polar mesosphere summer echoes (PMSE) have been carried out during summer 1994 in northern Norway using three radars on different frequencies: the ALOMAR SOUSY radar at Andenes on 53.5 MHz, the EISCAT VHF radar at Tromsø on 224 MHz and the MF radar at Tromsø on 2.78 MHz. During the common measuring period in July/August 1994, PMSE could be detected at 224 and 53.5 MHz, and there are strong hints that PMSE also occur at 2.78 MHz. Reliable correlations between hourly backscattered power values indicate that the PMSE structures have zonal extensions of more than 130 km and can be detected at very different scales (half wavelength) between 0.67 (EISCAT VHF radar) and 54 m (MF radar). Using the wind values derived by the MF radar it can be shown that the mesospheric wind field influences the structure of PMSE. The diurnal variation of PMSE is strongly connected with tidal-wind components, whereas spatial differences of PMSE can partly be explained by the mean wind field.

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