Articles | Volume 16, issue 23
Atmos. Chem. Phys., 16, 15135–15146, 2016
Atmos. Chem. Phys., 16, 15135–15146, 2016
Research article
07 Dec 2016
Research article | 07 Dec 2016

Comparison of retrieved noctilucent cloud particle properties from Odin tomography scans and model simulations

Linda Megner et al.

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Subject: Clouds and Precipitation | Research Activity: Atmospheric Modelling | Altitude Range: Mesosphere | Science Focus: Physics (physical properties and processes)
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Cited articles

Asmus, H., Robertson, S., Dickson, S., Friedrich, M., and Megner, L.: Charge balance for the mesosphere with meteoric dust particles, J. Atmos. Sol.-Terr. Phy., 127, 137–149,, 2015.
Bailey, S. M., Thomas, G. E., Hervig, M. E., and Lumpe, J. D.: Comparing nadir and limb observations of polar mesospheric clouds: The effect of the assumed particle size distribution, J. Atmos. Sol.-Terr. Phy., 127, 51–65,, 2015.
Bardeen, C. G., Toon, O. B., Jensen, E. J., Marsh, D. R., and Harvey, V. L.: Numerical simulations of the three-dimensional distribution of meteoric dust in the mesosphere and upper stratosphere, J. Geophys. Res., 113, D17202,, 2008.
Barth, C. A., Rusch, D. W., Thomas, R. J., Mount, G. H., Rottman, G. J., Thomas, G. E., Sanders, R. W., and Lawrence, G. M.: Solar Mesosphere Explorer: Scientific objectives and results, Geophys. Res. Lett., 10, 237–240,, 1983.
Baumgarten, G., Fiedler, J., Lübken, F.-J., and von Cossart, G.: Particle properties and water content of noctilucent clouds and their interannual variation, J. Geophys. Res.-Atmos., 113, D06203,, 2008.
Short summary
Noctilucent clouds (NLCs) are ice clouds that form at the polar summer mesopause and are very sensitive to temperature. They may therefore provide a way to monitor this remote region as our atmosphere changes. We show that temperature variations in the mesosphere are crucial for the growth of ice particles and that average fields are not enough to describe the process of NLC development. The paper also emphasises the difficulties in retrieving ice particle properties from optical observations.
Final-revised paper