Global observations of thermospheric lunar tidal winds

R. S. Lieberman, D. C. Fritts, N. Pedatella, E. Doornbos, D. A. Ortland

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Abstract

We present direct observations of the semidiurnal lunar tide zonal winds at 260km and 350km during low solar activity in 2007-2008, and 2010-2011. The migrating semidiurnal lunar tide, or M2, is a global feature with amplitudes of about 10ms-1 at equatorial latitudes, and 20ms-1 at high latitudes. Amplitude maxima appear twice yearly, between February and April and between August and November. M2 amplitudes during 2007-2008 are about 20% stronger than those during 2010-2011. These magnitudes are consistent with numerical predictions in WACCM-X. However, only one annual global-scale maximum is simulated during January-March.

Original languageEnglish
Pages (from-to)126-133
Number of pages8
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume136
DOIs
StatePublished - Dec 1 2015

Keywords

  • Lunar
  • Semidiurnal
  • Thermosphere
  • Tide

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