Diagnosing the Short-term Variability of Atmospheric Tides at the MLT
Region from Observations and a High Altitude Meteorological Analysis
System
Abstract
The variability of the middle atmosphere is driven by a variety of
atmospheric waves covering various spatial and temporal scales. In
particular, the northern winter mesosphere/ lower thermosphere at mid-
and polar-latitudes shows a huge variability related to planetary waves,
which can disturb the polar vortex leading to large scale coupling
effects like sudden stratospheric warmings (SSWs) altering the vertical
propagation conditions of tides and gravity waves. Here we are going to
investigate and diagnose the short time variability of tides (several
days) at the MLT using ground-based observations at mid and polar
latitudes and data from NAVGEM-HA for selected periods. NAVGEM-HA
provides information about the global structure of the zonal mean zonal
and meridional wind and the zonal mean temperature as well as the tides.
At mid- and high-latitudes the semi-diurnal tide (SW1 and SW2) is the
dominating tidal wave during the winter season, which is also seen in
meteor radar and lidar climatologies. Further, we analyze local meteor
radar and lidar observations at Andenes (polar-latitude) and Juliusruh
(mid-latitude) to diagnose the local amplitude and phase variability due
to changes in the background mean winds caused by planetary waves and
SSWs. We will show that the tidal phase (in UT) can drift significantly
within several days and weeks. These local measurements are also
compared to NAVGEM-HA applying the same diagnostic as to the
observations. In addition to the winter time observations, we will also
show results for the phase propagation of tides from summer periods.