The RMR lidar at Kühlungsborn

The Rayleigh-Mie-Raman lidar (RMR lidar) at Kühlungsborn is used for observation of temperatures and aerosol parameters of the atmosphere. The first RMR lidar has been in use between 1997 and 2013, measuring the following quantities:

  • nightly temperatures between 1 and 90 km altitude
  • nightly Noctilucent Clouds (NLC)
  • troposperic and stratospheric aerosols during day and night

Since 2010 a new RMR lidar is routinely in operation if weather allows. This lidar is optimized for soundings during the day and measures the followiing quantities:

  • temperatures between 40 and 90 km during the night and 40-75 km during the day
  • NLC during night and day
  • stratospheric aerosols up to 40 km altitude during the night

Especially the temperature and NLC soundings are unique. Together with the ALOMAR RMR lidar the lidar at Kühlungsborn is the most powerful lidar in the world for mesospheric observation during daylight. Below we describe the most important parts of the lidar. The principle of Rayleigh temperature retrieval is explained here.

The sender branch

The lidar sender mainly constist of a injection-seeded Nd:YAG laser with 30 pps and ~600 mJ pulse energy at 532 nm. The seed laser is locked to an iodine absorption line. By this, the long-term wavelength drift also of the pulsed laser is much below 0.1 pm. A 10x beam widening telescope is used to reduce the beam divergence to ~50 μrad. Behind that, different mirrors are used to guide the beam into the atmosphere. One of these mirrors is equipped with a fast and precise Piezo-mount, enabling an effective beam stabilisation. The beam stabilisation is required to guarantee the alignment between laser beam and receiver telescope field of view (FOV). The FOV is only ~60 μrad (~0.003°) and a misalignment may happen fast due to atmospheric turbulence and thermal drifts of the mirrors. Without beam stabilisation typically the alignment is lost completely after only a few minutes. For avoiding this the beam position is measured for every laser pulse by a CCD camera in the telecope . Differences from the desired position are measured and corrected within only a few milliseconds, i.e., before the next laser pulse.

The receiver branch

The receiver branch of the RMR lidar mainly consists of a 80 cm telescope with a focal length of ~3.2 m. The telescope serves simultaneously for lidar detection (90% of backscatter) and for beam stabilisation (10%). The FOV of the system is limited to ~60 μrad by a 0.2 mm quarz fiber. By the small FOV only limited amount of skylight is received - one of the prerequisites for daytime soundings.

The received light is collimated behind the fiber and passes different optical filters. These further reduce the unwanted skylight. Different filters are used:

  • interference filter with 130 pm spectral width,
  • first Fabry-Perot etalon with 4 pm spectral width,
  • second Fabry-Perot etalon with 4.5 pm spectral width.

The combination of small FOV and spectral filtering reduces the background by 1:10000, allowing for daytime soundings of temperatures up to 75 km altitude and detection of even weaks NLC.

The IAP RMR lidar at Kühlungsborn is widely automized. Human operators (typically hired university students) are mainly used for security reasons. Depending on weather between 1200 and 1500 h of data are aquiredeach year.

Selected publications

  • M. Gerding, J. Höffner, M. Kopp, R. Eixmann, and F.-J. Lübken, Mesospheric temperature and aerosol soundings during day and night: Spectral and spatial filtering techniques, 67-70, in Reviewed and revised papers at the 25th International Laser Radar Conference, St. Petersburg, Russia, 2010, 2010.
  • M. Gerding, G. Baumgarten, J. Höffner, J. Fiedler, R. Eixmann, and F.-J. Lübken, Temperature and aerosol soundings in the middle atmosphere at different mid and high-latitude Lidar stations during day and night, in Remote Sensing of Clouds and the Atmosphere XIV, R. H. Picard (Ed.), Proc. SPIE, Vol. 7475 (SPIE, Bellingham, WA), 74750A-1-74750A-12, 2009.


Dr. Michael Gerding

Sounding overview

Here you can find an overview on the available sounding periods.

RMR lidars Kühlungsborn

IAP building with laser beams of new and old RMR lidar

Lidar receiver

Receiver parts of the new RMR lidar