The Bubble Lab is an experimental laboratory to study bubble processes in hydrothermal and volcanic terrain. Earthquake and volcano processes are commonly accompanied by migration of fluids and deformation of fluid systems and their interaction with the host rock, including fracturing, fluid-filled crack growth and diking. The coupling between fluids and rock works in both ways: On one side, changes in the state of fluid-rock systems are thought to encourage or discourage tectonic earthquakes, …

Simulating geodynamic processes is a challenging task because of the non-linearity and cross-scale nature of tectonic processes. A great challenge is the multispectral character of lithosphere deformation ranging from earthquake rupture (seconds) to tectonic evolution (Millions of years). At the same time, deformation mechanisms determined at the micro-scale (rock friction and crystal plasticity) are responsible for the motion and internal deformation of tectonic plates. This requires a …

The groundwater monitoring is used to evaluate the local quality and quantity of the groundwater. These information are required to obtain important insights in the hydrochemical processes in the aquifer, as well as the origin and residence time of groundwater.
The Grundfos MP 1 submersible pump set with a connected, closed flow cell enables observations of the physicochemical parameters with digital IDS sensors (temperature, pH, electrical conductivity, redox potential, dissolved oxygen), …

The MSF-Lab, established in 2004, is part of the Department of Experimental Planetary Physics and is used for different astrobiological and physical experiments to simulate the key environmental conditions like pressure, temperature, radiation, gas composition, and primarily also the diurnally varying atmospheric humidity in a range from earth conditions to similar to those at the near-surface atmosphere of Martian mid- and low latitudes. A further part of the laboratory are tests with gas, …

The Planetary Analog Simulation Facility-Laboratory (PASLAB) at the DLR is used for different astrobiological, chemical and physical experiments to simulate variations in key environmental conditions like pressure, temperature, radiation and gas composition, under conditions ranging from Earth-like (including Early Earth) to the near-surface atmosphere of Martian mid- and low latitudes and exoplanets (e.g. temperature range between -70 °C to +20 °C, low pressures 6 to 10 mbar, etc.). The DLR …