Institute of Meteorology and Climate Research

MIPAS provides first observational evidence of the coupling from the lower atmosphere to the thermosphere during a major stratospheric warming

 

 

The figure shows the temperature evolution of the Arctic polar winter atmosphere (70N - 90N) during the unprecedented major stratospheric warming in January 2009 in the altitude range from 20 to 170 km. The stratospheric warming (red, between 20 and 50 km) is accompanied by a mesospheric cooling (blue, between 80 and 100 km) and a thermospheric warming (yellow to red, between 100 and 150 km). This is the first observational evidence of a dynamical coupling of the lower atmosphere and the thermosphere in the 120–150 km range by means of satellite data.

We used temperature data from the Michelson Interferometer for Passive Atmospheric Sounding on board ESA's Envisat satellite to analyze the temperature responses in the mesosphere and thermosphere up to 170 km to a major stratospheric sudden warming (SSW) which occurred in January 2009. The temperature observations show clear signatures of a mesospheric cooling and a thermospheric warming, the latter peaking at 120–140 km in agreement with model predictions. From the analysis of the zonal temperature structure during the SSW a pronounced wave 1 pattern was found in the entire middle and upper polar atmosphere with maximum amplitudes around 50 and 140 km. In the mesosphere, the wave amplitude is significantly damped. The wave amplification above is most likely produced by in situ forced planetary waves in the mesosphere and lower thermosphere region.

Temperature in the upper atmosphere is retrieved from CO2 lines up to ~100 km, and above 100 km from NO lines under local thermodynamic dis-equilibrium, together with the NO volume mixing ratio.

The observational data have been recorded by MIPAS in its Upper Atmosphere observation mode which covers the altitude range of 40 to 170 km. Since end of 2007, MIPAS observes the Upper Atmosphere regularly every tenth day, and thus provides monitoring of dynamical processes and the solar impact on the atmosphere.

For further details see:
http://www.agu.org/pubs/crossref/2010/2010GL043619.shtml
http://www.agu.org/pubs/crossref/2005/2004JD005225.shtml
http://www.agu.org/pubs/crossref/2000/1999JD900822.shtml