IAP Kühlungsborn

Noctilucent cloud (NLC)

Noctilucent clouds (NLC) exist at the edge of space and consist of ice particles that are only a few 10 nm small. So they are less than 1/10 of the wavelength of light or less than 1/100 of a dust particle. How big the particles are in detail, but also how many particles occur per volume, is the subject of intensive research. In particular, the water content of the cloud is important for understanding NLC.
In addition to understanding the formation of clouds we can investigate processes in the upper atmosphere just from monitoring the clouds. Most of the processes can not be explored and understood otherwise. Since the cloud particles are so tiny, they follow the movement of the air, at least for a short time almost completely. Only when the icy particles in the clouds are moved for several minutes or several kilometers, the microphysical changes of the particles must be considered.

NLC are observed with lidar (active) or cameras (passive), sounded in-situ by rocket-borne instruments, but also simulated using combined microphysical and dynamical models. On the observational side modern cameras allow, studying the motion in a cloud with 10 m accuracy even when the cloud is about 500 km away. With such a fine resolution the transition from secondary wave motion to turbulence e.g. in Kelvin-Helmholtz instabilities is measured. Planetary scales of many 100 km are investigated using satellite data and 3-D simulations of the atmosphere and the microphysics of ice. The combination of measurement and modeling of the nanometer scale NLC particles thus helps to improve our understanding of the dynamic processes at the edge of space from scales of a few meters to hundreds of kilometers.

Selected publications

  • Gerding, M., J. Zöllner, M. Zecha, K. Baumgarten, J. Höffner, G. Stober and F.-J. Lübken, Simultaneous observations of NLC and MSE at midlatitudes: Implications for formation and advection of ice particles, Atmos. Chem. Phys., 18, 15569–15580, doi: 10.5194/acp-18-15569-2018, 2018
  • G. Baumgarten and D. C. Fritts, Quantifying Kelvin-Helmholtz instability dynamics observed in Noctilucent Clouds: 1. methods and observations, J. Geophys. Res., 9324–9337, doi:10.1002/2014JD021832, 2014.
  • J. Fiedler, G. Baumgarten, U. Berger, A. Gabriel, R. Latteck, and F.-J. Lübken, On the early onset of the NLC season 2013 as observed at ALOMAR, J. Atmos. Solar-Terr. Phys., 2014.
  • M. Gerding, M. Kopp, P. Hoffmann, J. Höffner, and F.-J. Lübken, Diurnal variation of midlatitude NLC parameters observed by daylight-capable lidar and their relation to ambient parameters, Geophys. Res. Lett., 40, 6390-6394, doi:10.1002/2013GL057955, 2013.
  • N. Kaifler, G. Baumgarten, J. Fiedler, and F.-J. Lübken, Quantification of waves in lidar observations of noctilucent clouds at scales from seconds to minutes, Atmos. Chem. Phys., 13, 11757-11768, doi:10.5194/acp-13-11757-2013, 2013.
  • F.-J. Lübken, U. Berger, J. Kiliani, G. Baumgarten, and J. Fiedler, Solar variability and trend effects in mesospheric ice layers, in Climate And Weather of the Sun-Earth System (CAWSES): Highlights from a priority program, Springer, F.-J. Lübken, Dordrecht, The Netherlands, doi:10.1007/978-94-007-4348-9, 2012.


Dr. Gerd Baumgarten