Articles | Volume 10, issue 8
Atmos. Meas. Tech., 10, 2989–3006, 2017
Atmos. Meas. Tech., 10, 2989–3006, 2017

Research article 21 Aug 2017

Research article | 21 Aug 2017

Comparison of global datasets of sodium densities in the mesosphere and lower thermosphere from GOMOS, SCIAMACHY and OSIRIS measurements and WACCM model simulations from 2008 to 2012

Martin P. Langowski1, Christian von Savigny1, John P. Burrows2, Didier Fussen3, Erin C. M. Dawkins4,5, Wuhu Feng6,7, John M. C. Plane6, and Daniel R. Marsh8 Martin P. Langowski et al.
  • 1Institute of Physics, Ernst Moritz Arndt University of Greifswald, Greifswald, Germany
  • 2Institute of Environmental Physics, University of Bremen, Bremen, Germany
  • 3Belgian Institute for Space Aeronomy, Brussels, Belgium
  • 4NASA Goddard Space Flight Center, Greenbelt, MD, USA
  • 5Department of Physics, Catholic University of America, Washington, DC, USA
  • 6School of Chemistry, University of Leeds, Leeds, UK
  • 7National Center for Atmospheric Science, School of Earth and Environment, University of Leeds, Leeds, UK
  • 8National Center for Atmospheric Research, Boulder, CO, USA

Abstract. During the last decade, several limb sounding satellites have measured the global sodium (Na) number densities in the mesosphere and lower thermosphere (MLT). Datasets are now available from Global Ozone Monitoring by Occultation of Stars (GOMOS), the SCanning Imaging Absorption spectroMeter for Atmospheric CHartography (SCIAMACHY) (both on Envisat) and the Optical Spectrograph and InfraRed Imager System (OSIRIS) (on Odin). Furthermore, global model simulations of the Na layer in the MLT simulated by the Whole Atmosphere Community Climate Model, including the Na species (WACCM-Na), are available. In this paper, we compare these global datasets.

The observed and simulated monthly averages of Na vertical column densities agree reasonably well with each other. They show a clear seasonal cycle with a summer minimum most pronounced at the poles. They also show signs of a semi-annual oscillation in the equatorial region. The vertical column densities vary from 0. 5  ×  109 to 7  ×  109 cm−2 near the poles and from 3  ×  109 to 4  ×  109 cm−2 at the Equator. The phase of the seasonal cycle and semi-annual oscillation shows small differences between the Na amounts retrieved from different instruments. The full width at half maximum of the profiles is 10 to 16 km for most latitudes, but significantly smaller in the polar summer. The centroid altitudes of the measured sodium profiles range from 89 to 95 km, whereas the model shows on average 2 to 4 km lower centroid altitudes. This may be explained by the mesopause being 3 km lower in the WACCM simulations than in measurements. Despite this global 2–4 km shift, the model captures well the latitudinal and temporal variations. The variation of the WACCM dataset during the year at different latitudes is similar to the one of the measurements. Furthermore, the differences between the measured profiles with different instruments and therefore different local times (LTs) are also present in the model-simulated profiles. This capturing of latitudinal and temporal variations is also found for the vertical column densities and profile widths.

Short summary
Meteoric metals form metal layers in the upper atmosphere anandplay a role in the formation of middle-atmospheric clouds and aerosols. However, the total metal influx rate is not well known. Global Na datasets from measurements and a model are available, which had not been compared yet on a global scale until this paper. Overall the agreement is good, and many differences between measurements are also found in the model simulations. However, the modeled layer altitude is too low.