Details

Autor(en) / Beteiligte

• Liu, H.-L.
• Li, T.
• She, C.-Y.
• Oberheide, J.
• Wu, Q.
• Hagan, M. E.
• Xu, J.
• Roble, R. G.
• Mlynczak, M. G.
• Russell III, J. M.

Titel

Comparative study of short-term diurnal tidal variability

Ist Teil von

• Journal of Geophysical Research - Atmospheres, 2007-09, Vol.112 (D18), p.D18108-n/a

Ort / Verlag

Washington, DC: American Geophysical Union

Erscheinungsjahr

2007

Quelle

Wiley Online Library All Journals

Beschreibungen/Notizen

• The wind and temperature measurements from an unusually long period operation of the sodium lidar at Colorado State University (41°N, 105°W) around September equinox 2003 showed significant short‐term tidal variability. Coincident with the large tidal changes, a strong temperature inversion layer was also observed above 90 km. Examination of the simultaneous temperature measurement from the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument, on board the Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite, not only confirms the existence of the inversion layer but also reveals the global nature of the inversion, suggesting the presence of a transient planetary wave in the mesosphere. The large tidal variability, therefore, is probably a consequence of the interaction between the transient planetary wave and tides. This possibility is investigated by using the NCAR thermosphere‐ionosphere‐mesosphere‐electrodynamics general circulation model (TIME‐GCM) and by comparing model results with the lidar, SABER, and TIMED Doppler Interferometer (TIDI) measurements. With a large transient planetary wave specified at the model lower boundary, the model is able to produce strong diurnal tidal variability comparable to that from the lidar observation, and the modeled temperature inversion is similar to that from the SABER measurement. The model results suggest that the planetary/tidal wave interaction excites nonmigrating tides and modulates the gravity modes and/or the rotational modes of the diurnal migrating tide. Among the nonmigrating tides, the diurnal zonally symmetric (S = 0) component is the strongest, and its interaction with the planetary wave leads to a strong diurnal eastward wave number 1 component.