In the last ten years a total of 25 sounding rock: ets employing ionization
gauges have been launched at high latitudes (similar to 70 degrees N) to m
easure total atmospheric density and its small scale fluctuations in an alt
itude range between 70 and 110 km. While the determination of small scale f
luctuations is unambiguous, the total density analysis has been complicated
in the past by aerodynamical disturbances leading to densities inside the
sensor which are enhanced compared to atmospheric values. Here, we present
the results of both Monte Carlo simulations and wind tunnel measurements to
quantify this aerodynamical effect. The comparison of the resulting 'ram-f
actor' profiles with empirically determined density ratios of ionization ga
uge measurements and falling sphere measurements provides excellent agreeme
nt. This demonstrates both the need, but also the possibility, to correct a
erodynamical influences on measurements from sounding rockets.
We have determined a total of 20 density profiles of the mesosphere-lower-t
hermosphere (MLT) region. Grouping these profiles according to season, a li
sting of mean density profiles is included in the paper. A comparison with
density profiles taken from the reference atmospheres CIRA86 and MSIS90 res
ults in differences of up to 40%. This reflects that current reference atmo
spheres are a significant potential error source for the determination of m
ixing ratios of, for example, trace gas constituents in the MLT region.