AWIPEV Atmosphere Observatory

At the AWIPEV Atmosphere Observatory, long-term measurements of atmospheric thermodynamics, clouds, aerosols and trace gases are operated.

Information on the respective AWI long-term observation (LTO) data series is described here.

 
InstrumentPhotoRetrieved ParametersDescription of InstrumentationMore information
Weather masttemperature, relative humidity, wind direction, wind speed in 2 and 10 m above groundPT100 temperature sensors, Vaisala XXX humidity sensors, and Thies Clima classic combined wind sensors are installed in 2 and 10 m above ground.RiS Project 6817
>> Data
Surface radiation Net radiation components (SW up, SW down, LW up, LW down), direct and diffuse radiation Ventilated CMP22 pyranometers, CGR4 and Eppley PIR pyrgeometers monitor the downward and upward radiation components. Ris Project 2350
The measurements contribute to the Baseline Surface Radiation Network (BSRN). Data are accessible upon registration with BSRN (www.bsrn.awi.de)
Ceilometer Cloud base height Pulsed 910nm diode laser instrument (Vaisala CL51) that detects the base height of cloud layers up to 13 km. RiS Project 6817
>> Data
Radiosonde Vertical profiles (0 - 30km) of temperature, pressure, relative humidity, wind speed and direction The radiosonde (Vaisala RS41) ascents with a helium-filled balloon while transmitting the measured data to the ground station. RiS Project 1118
>> Data
The Ny-Alesund radiosonde data also contribute to the GCOS Reference Upper-Air Network [GRUAN].
Ozone sonde Vertical profiles (0-30 km) of ozone concentration The ozone concentration is detected by an electrochemical cell passed through by a defined flow of ambient air. The ozone sonde is launched together with a radiosonde on a helium-filled balloon. RiS Project 1322
The data contribute to the Network for the Detection of Atmospheric Composition Changes (NDACC).
>> Data
Sun Photometer Aerosol optical depth The sun photometer is a small telescope that automatically tracks the sun in absence of clouds. It measures the aerosol optical depth (AOD) in several wavelengths between 360nm to 1024nm. RiS Project 2353
>> Data
Star Photometer Aerosol optical depth (during polar night) The star photometer is a telescope that uses star light during the dark season to measure the aerosol optical depth (AOD) in several wavelengths. RiS Project 2353
>> Data
"KARL" Koldewey Aerosol Raman Lidar Vertical profiles of aerosol backscatter coefficient A pulsed laser is emitted to the atmosphere where the light is scattered back by small particles (aerosols) and droplets. RiS Project 2399
More information on the instrument and related research is provided here
Micropulse Lidar (MPL) Vertical profiles of aerosol and cloud particle backscatter A pulsed laser is emitted to the atmosphere where the light is scattered back by small particles (aerosols) and droplets. RiS Project 3186.
The data contribute to the NASA Micro-Pulse Lidar Network (MPLNET).
>> Data
Doppler Lidar (WindCube) Vertical profiles of wind (up to ~1km) The wind lidar uses particles (aerosol, clouds) as a tracer to measure the wind. It runs automatically 24/7 and provides the 3D wind field up to approx. 1km altitude. However, the effective range depends on the visibility.RiS Project 6525 .
> Quick look for tropospheric wind
>> Data
Microwave Radiometer (HATPRO) Temperature and humidity profiles in the troposphere, liquid water path Passive microwave radiometer that continuously measures profiles of the temperature and the water vapour. While the temporal resolution is about 10minutes, the vertical resolution is coarser than a radiosonde. RiS Project 6525
> Quick look for Relative Humidity.
> Quick look for Temperature
>> Data
35 GHz Cloud Radar macro- and microphysical cloud properties The 35 GHz cloud radar data are synergetically analyzed in combination with precipitation observations and other collocated instrumentation. RiS Project 10523.
The cloud radar measurements are performed in collaboration with the University of Cologne. Data are processed with the syncloud algorithm.
> Quick look for 35GHz cloud radar data
94 GHz Cloud Radar macro- and microphysical cloud properties The 94 GHz cloud radar data are synergetically analyzed in combination with precipitation observations and other collocated instrumentation. RiS Project 10523.
The cloud radar measurements are performed in collaboration with the University of Cologne. Data are processed with the syncloud algorithm.
> Quick look for 94GHz cloud radar data

>> Data

The data contribute to > CLOUDNET
Micro Rain Radar (MRR) precipitation rate, liquid water content, drop size distribution The zenith pointing MRR is operating at 24 GHz and detects precipitation in the lowermost kilometer of the atmosphere. RiS Project 10523.
The micro rain radar measurements are performed in collaboration with the University of Cologne.
> Quick look for MRR data

>> Data
Laser Precipitation Disdrometer size and speed of falling precipitation particles The data of the Parsivel laser disdrometer allow to calculate the type, amount, intensity and kinetic energy of the precipitation, the visibility in the precipitation, and the equivalent radar reflectivity. RiS Project 10523.
The disdrometer measurements are performed in collaboration with the University of Cologne.
>> Data
Video in situ Snowfall Sensor (VISSS) snow particle size, shape, and mass distribution Falling particles are observed by two cameras at a 90° angle with high resolution, consquent data processing allows sizing, matching and tracking individual particles. RiS Project 11763.
The snowfall in-situ measurements are performed in collaboration with the University of Leipzig.
Radiometer for Atmospheric Measurements (RAM) Vertical profiles of O3 and CO in the upper stratosphere Passive millimeterwave radiometer to continuously measure highly resolved spectra of the O3 and CO emission lines at 142 and 230 GHz, respectively. RiS Project 390.
The RAM measurements are performed in collaboration with the University of Bremen, see external project page
Fourier Transform Infrared Spectrometer (FTIR) Atmospheric trace gases, e.g. CO, CH4, O3 With FTIR spectroscopy, emission spectra of the atmosphere are obtained to examine the variation of trace gases. RiS Project 6047.
The FTIR measurements are performed in collaboration with the University of Bremen, see
external project page
> Quick Look