Synergetic use of instruments and models
About
The synergy of new instrumentation for observing the atmosphere with modeling of the atmosphere from physical principles and with evaluating data by machine learning and artificial intelligence (AI) is a key strength of ICE-4. For example, global circulation models are an important tool to gain understanding of the complex and chaotic processes within our atmosphere. These models contain always approximations, which require tuning by observational data. Novel predictive models based fully on machine learning require even more observational data to become reliable. Other numerical models are designed to simulate very specific physics within the atmosphere such as emission and absorption of light, the formation of clouds or the propagation of atmospheric waves. To further our understanding of these processes, novel instruments measuring the atmosphere are needed that provide the required data from aircraft, balloons, or satellites. Measurement platforms such as zero-pressure balloons going up to 35 km altitude or the German research aircraft HALO allow our instruments to have a close look at one of the last frontiers that are surprisingly unknown. Today, novel observations still uncover new atmospheric phenomena and chemical reactions that are missing in modelling efforts. Such new observations then in stigate a flurry of activities in the scientific community that often result in better forecasts of weather, boundary layer pollution, or extreme weather events.
For example, one still open question is the general speed of atmospheric large-scale turn-over. Due to its slowness, it is very difficult to measure this circulation directly. However, the stratospheric circulation has profound impact on long-term climate forecasts. We use stratospheric balloons carrying our GLORIA and air-core instruments, or satellite-borne remote sensing instruments to measure highly accurate trace gas concentrations of long-living anthropogenic substances. Combining these unique measurements with the predictions of our global-circulation model CLaMS for different configurations, one can derive estimates about both the current speed of the circulation as well as determine whether or not this circulation system is in the process of change.
Research Topics
Our institute uses many different models and maintains a wide range of unique measurement instruments. Here is an incomplete list:
- The Chemical Lagrangian Model of the Stratosphere (CLaMS), together with the coupled ECHAM MESSy Atmospheric Chemistry (EMAC) model, is being developed and used to examine a wide variety of scientific questions in the upper troposphere and lower stratosphere.
Read more... - We operate a suite of measurement instruments on mini-balloons, i.e. normal ”weather balloons”, which are costeffective and can be launched from many placed.
Read more... - The research aircraft HALO (High Altitude and Long Range Research Aircraft) provides an excellent combination of high flight altitude and long range for investigations of climate processes in the UTLS. Beside GLORIA, we operate the FISH and AMICA instruments on this platform.
Read more... - The Global Radiance Imager for the Atmosphere (GLORIA) is an air-borne infrared limb sounder, which can tomographically measure temperature (and thereby gravity waves) as well as many trace gas species. It serves as an airborne demonstrator for the Earth Explorer 11 candidate mission CAIRT.
- We develop the Juelich Rapid Spectral Simulation Code (JURASSIC2), a radiative transfer model, mainly to evaluate measurements by satellite- and air-borne spectrometers, such as our GLORIA or the ESA FORUM instrument, with a focus on tomographic studies.
- Analyzing gravity waves in three-dimensional data from either observations or measurements is a challenge due to the localized nature of the waves above strong source regions and the rapid change of wave parameters in shear zones.
Read more... - FUNMASS (Caribic)