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Institute of Astronautics | Prof. Dr. rer. nat. U. Walter
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Accelerator Laboratory

The Institute has extensive laboratory equipment to conduct experimental tasks in the field of micrometeoroid simulation and dust research. A plasmadynamic high-velocity accelerator (particle size: 20 µm up to approx. 100 µm; speeds of up to approx. 12 km/s), an electrothermal accelerator (projectiles up to 30 mg, speeds of up to 5.5 km/s) and an electromagnetic accelerator (particles with a mg range; speeds of <500 m/s) are available for particle acceleration. The capacitor banks required for operating the individual accelerators have a capacity of 352 µF, 60 µF and 10 µF, and they provide the corresponding surge currents of up to 450 kA, 100 kA and 30 kA. The samples are bombarded in vacuum tanks with a vacuum of max. 10-5 mbar. The largest tank is equipped with a length of 85 cm and a diameter of 80 cm.

The measuring technology required for operation and control of the accelerator facilities comprises high-voltage sensing heads (up to 40 kV), high-current probes (up to 500 kA), pressure gauges (up to 6 kbar) and high-speed photography (single frame with exposure time of at least 10 ns).

A small scanning electron microscope, different optical microscopes, a contactless 3D surface analyser as well as a microhardness tester are available for the analysis of the bombarded samples. Sensitive samples can be handled on a clean-room workbench.

The experimental tasks are supported by a precision-engineering workshop, which has extensive metal working possibilities, as well as by an electronic workshop. We have specific skills for manufacturing vacuum and high-voltage components (e.g. high-current vacuum bushings, magnetic field probes, Rogowski coils).

In the following you will find some examples of projects to illustrate the laboratory work:

ICAPS - Technology Support with Dust Experiments under Microgravitation

The experiment proposal ICAPS (Interactions in Cosmic and Atmospheric Particle Systems) is an international research programme under the leadership of ESA and refers to experiments with small particles in weightlessness. A large number of technological problems need to be solved to be able to implement the experimental platform at the International Space Station. The Institute of Astronautics develops concepts and engineering models especially in the fields of handling, transporting, and accelerating the micro-dust particles that are necessary for the experiments.

The physical interactions of particles with each other, with gas, and light are important in a large number of scientific questions. Within the framework of the experiment proposal ICAPS six areas have been qualified central scientific issues, like aerosol physics, the simulation of regolith, or the agglomeration of dust particles. The latter scientific focus is critically important to understand how our solar system was formed. It is assumed that the planets formed out of a dense gas-dust slice around the new-born sun. When these so-called protoplanetesimals are very small (< 1 km), it is assumed that the main process of planetary growth is the dust agglomeration (collision of dust particles with subsequent adhesion). Under the management of Prof. Jürgen Blum (formerly Jena University; now Technical University Brunswick) experiments regarding the investigation of dust clouds and particle agglomerates are carried out. The simulation material is glass balls with a typical diameter of 1 micron. As these micro-particles are susceptible to clogging, deagglomeration mechanisms have to be developed, that also work under conditions of vacuum and weightlessness. The Institute of Astronautics developed such a deagglomeration and dust injection device on the basis of the turbo-molecular pump (very fast rotating blade wheels). The picture shows a dust agglomerate created with this device at the Astrophysical Institute of the Jena University.

The Institute of Astronautics also works on other tasks related to ICAPS. These tasks are the automated handling of microparticles, and the defined generation of macroscopic dust agglomerates. Dust cakes with a size of some ccm need to be handled and produced reproducibly especially for planned research on regolith. The goal is to produce loose structures that would break down on Earth because of their own weight.

HVL Development - Development of High Velocity Launchers

About 30 years ago a plasmadynamic accelerator for the simulation of micrometeoroids was set up at the Institute of Astronautics. Since that time, the accelerator principle has been further developed and its capacity increased. On the basis of the insights and skills gained during this period the Institute has developed, build and operated further high-capacity accelerators. These accelerators work according to the electrothermal, electromagnetic, or electrodynamic principle; and they have one thing in common: their energy source is a capacitor bank.

Plasmadynamic particle accelerator:
More than 25 years ago the Institute started building a high-velocity accelerator to simulate micrometeoroids and space debris. This accelerator has been improved, upgraded and supplemented with new components. The plasmadynamic accelerator installation can accelerate particles with a diameter of about 30 µm up to 100 µm until they reach a speed of a little bit more than 12 km/s. The particles that are used are glass balls, which are aerodynamically accelerated by means of a very fast plasma jet. The plasma jet is generated and accelerated by ionising injected He gas in a coaxial arrangement of electrodes (diameter: 33 mm; length: 160 mm). This is done with a surge current discharge of a capacitor bank (capacity: 352 µF). A charging voltage of the capacitor bank of up to 16 kV leads to peak currents of up to 450 kA. At the end of the coaxial electrode arrangement the plasma is compressed in a self-excited conical coil (compressor coil). This plasma jet, which has been bundled, interacts with the quiescent microparticles and accelerates them. The picture above shows the arrangement of electrodes with the compression coil.
The accelerator is operated in a vacuum tank (diameter: 85 cm; length: 220 cm). This tank is connected with the impact chamber (diameter: 90 cm; length: 80 cm) by means of a tube. This chamber can be evacuated to up to 10-5 mbar. Typical fields of application of this accelerator are the simulation of micrometeoroids, basic research on high-velocity impacts, and the calibration of space experiments for dust research.

Electrothermal Particle Accelerator:
The accelerator is based on the following principle: Energy saved in a capacitor bank (60 µF; 12 kV) is used in order to generate a high pressure plasma (up to 10 kbars) between two electrodes by means of a current discharge in a very narrow capillary (length: 20 to 40 mm). One of the two electrodes is formed as a barrel (diameter: 4 mm) with a projectile of the same calibre. The high plasma pressure in the capillary accelerates the projectile. Maximum speeds of up to 5.5 km/s were achieved in the vacuum for projectile masses of approx. 25 mg. These are extremely good figures for a single-stage accelerator. Although we have to use a new barrel and a new capillary for every experiment in order to achieve these speeds (because of component erosion caused by the plasma), the accelerator is characterised by a relatively easy use with very different applications (like demonstration accelerators for teaching; impact research in heat shields; DOD research in turbine blades; impact experiments in water ice).

Electromagnetic Accelerator:
The eddy-current accelerator is very easy to use in order to accelerate any dust particles to a speed of some hundred m/s. The strong change of current during the discharge of a capacitor bank by means of the accelerator coil generates a vigourously changing magnetic field in the coil. A thin aluminium slice is placed above the coil (e.g. d = 30 mm, t = 0,5 mm); a current is induced in this slice which produces a field opposed to the original magnetic field and thus leads to the acceleration of the aluminium slice. In the centre of the slice (sabot) is a centre punch to take up the projectile. Sabot and projectile are accelerated together; the sabot is kept back by a massive stopper, whereas the projectile continues moving in the direction of the experiment. If the projectiles are too heavy, the aluminium slice is destroyed under very high accelerations (typically 10 6 g) because of the high inertia force of the projectile. The shape of the sabot was optimised during the last two years, which led to a considerable efficiency increase of the accelerator. Steel balls with a diameter of 2.5 mm can be accelerated reliably to up to 280 m/s.
Typical applications for this accelerator are basic research with low impact speeds, research of dust adhesion, and the simulation of abrasive particles in jet engines.

Presentation Laboratory
Presentation Laboratory (PDF file)
Presentation Fast Dust and Small Particles (PDF file)
 

 

Semester und Diplomarbeiten
 
Title: Analyse der Housekeepingdaten im Jahr 1998 des Weltraumexperiments MDC auf der japanischen Mission NOZOMI
  Semester Thesis - Theoretical - RT-SA 04/15
The Housekeepingdata of the Mars Dust Counter (MDC) received in 1998 are examined and analysed. The task is to look for patterns characterizing the probability of data recording and for correlations of the data with interplanetary events in 1998. The MDC, developed and buitl by the TUM, was one of 15 experiments ...
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Title: Charakterisierung des Rauschverhaltens am Mars Dust Counter
  Semester Thesis - Theoretical - RT-SA 03/07
This theoretical term paper analyses the noise behaviour at the Mars Dust Counter (MDC). The Mars Dust Counter is a micrometeoroids detector, which is installed at the Japanese satellite NOZOMI. In the first chapter the presence of micrometeoroids is described. Further the satellite NOZOMI, the structure of the MDC and...
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Title: MDC BremSat Datenanalyse
  Semester Thesis - Theoretical - RT-SA 04/18
In the context of this semester paper an analysis of the MDC BremSat data is accomplished. These data were collected 1994 during the BremSat mission by the MDC in the near earth orbit. The evaluation essentially consists of an iterative selection of actual impact particles selected out of the existing 11683 signa...
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Title: On-Board Software Upgrade of the Space Experiment Mars Dust Counter
  Master Thesis - Experimental - RT-DA 03-15
As sensor data output is more and more increasing, modern space probe missions beyond Earth orbit are demanding better data compression techniques to transmit the huge information loads. Moreover, if a severe degradation of downlink capability occurs, the fate of the whole mission can depend on improved compress...
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Title: Signalklassifikation mit Neuronalen Netzen
  Semester Thesis - Theoretical - RT-SA 03-06
Since 1998 the interplanetary experiment Mars Dust Counter of the Institute of Astronautics (LRT) at the Technische Universität München transmits data to the LRT, where the data are analysed. In this study a system is presented which is able to classify signals by using a neural network. This neural net...
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Title: Validation of the Software Update on MDC NOZOMI with the MDC HITEN Data
  Semester Thesis - Theoretical - RT-SA 04/17
The Munich Dust Counter was a scientific space mission on the Japanese satellite HITEN. The experiment is a plasma dust counter developed and built by the Institute of Astronautics (LRT) at the Technical University of Munich. The mission was the first of a total of three successful cosmic dust counters. The data that w...
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