Longitudinal MLT wind structure at higher mid-latitudes as seen by meteor radars at central and Eastern Europe (13°E/49°E)

Dmitriy Korotyshkin, Eugeny Merzlyakov, Christoph Jacobi, Friederike Lilienthal, Qian Wu

Research output: Contribution to journalArticlepeer-review

9 Scopus citations

Abstract

The mid-latitude mesosphere and lower thermosphere (MLT) wind speeds measured by two SKiYMET meteor radars (MRs) at Collm (51°N, 13°E) and Kazan (56°N, 49°E) during 2016–2017 were analyzed to study longitudinal wind structures. The differences between monthly mean prevailing wind speeds and tidal amplitudes were compared with the corresponding differences obtained from TIMED/TIDI satellite winds and gradient wind speeds from the AURA/MLS instrument. It is shown that the MR wind difference between the two sites is statistically significant. The difference of the horizontal prevailing winds can be explained by a superposition of the background zonal flow, which is different at the two latitudes, with stationary planetary waves of different origin. Non-migrating tides contribute significantly to the difference of the semidiurnal tidal winds between the two sites.

Original languageEnglish
Pages (from-to)3154-3166
Number of pages13
JournalAdvances in Space Research
Volume63
Issue number10
DOIs
StatePublished - May 15 2019

Keywords

  • Mesosphere and lower thermosphere
  • Migrating tide
  • Non-migrating tides
  • Prevailing wind
  • Stationary planetary waves

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