The specialized course in Astronomy and Astrophysics offers an advanced labwork. The experiments will take place at section Astronomy (Sand 1) or at section Computational Physics (Auf der Morgenstelle 10). The experiments in Nuclear Physics for students of Master Astro and Particle Physics will take place at Physikalisches Institut (Auf der Morgenstelle 14).
In SS 2019 the labwork will be held as block during semester break from 29.07. - 16.08.2019 (extended) (Mo, We, Fr 9:00-18:00). If there should occur overlaps with other courses or tests, single experiments might be shifted to later dates in agreement with the corresponding tutor.
Preparatory meeting (arrangement of groups, discussion of possible scheduling conflicts): Tu. 23.07.2019, 9:00 Uhr, Astronomy, Sand 1, lecture hall A 104 (orientation map, room map)
If you are unable to attend the preparatory meeting, you should register in advance by e-mail with Jürgen Barnstedt (or via Ilias, see below). A personal appointment for a preparatory meeting will be arranged.
Link for direct registration by ILIAS: https://ovidius.uni-tuebingen.de/ilias3/goto.php?target=crs_1952663_rcode4QkFedUJJQ&client_id=pr02
In WS 2019/20 the labwork will be held as block during semester break from 10.02. - 21.02.2020 (Mo, We, Fr 9:00-18:00). If there should occur overlaps with other courses, single experiments might be shifted to later dates in agreement with the corresponding tutor.
Preparatory meeting (arrangement of groups, discussion of possible scheduling conflicts): Tu. 04.02.2020, 9:00 Uhr, Astronomy, Sand 1, lecture hall A 104 (orientation map, room map)
- X-ray--CCD (Astronomy, Thomas Schanz room A142, meeting place room A112)
Estimation of properties of a pn-CCD in the lab, analysis of measurements with the X-ray satellite XMM-Newton. (experiment instructions; poster (outdated), poster of the eRosita project).
- MCP detectors (Astronomy, Jürgen Barnstedt room A121, meeting place room A121)
Using the micro channel plate detector of the ORFEUS echelle spectrometer the working principle and the properties of such detectors will be analyzed. (experiment instructions; poster)
- Instruments of the gamma astronomy - RMC (Astronomy, Gerd Pühlhofer room A218, meeting place in front of room A110)
Laboratory measurements with an imaging Rotating Modulation Collimator (RMC) by using radioactive sources. (experiment instructions (german); poster) - Note: As the expriment will take place in the basement, it is advisable to wear warm clothing, even in midsummer!
- Digital electronics for X-ray and gamma detectors (Astronomy, Chris Tenzer room A107, meeting place in front of room A107)
Setup of a data aquisition electronics by means of programmable electronic components - FPGAs. (experiment instructions) - Note: As the expriment will take place in the basement, it is advisable to wear warm clothing, even in midsummer!
- Photometry and spectroscopy (Astronomy, Thomas Rauch room A211, meeting place room A211)
Solar and stellar spectroscopy and color-brightness-diagrams. (experiment instructions; poster)
- Radio astronomy (Astronomy, Victor Doroshenko room A219, meeting place room A105)
Measuring of the milky way by means of the 21cm radio emission of hydrogen, generation of a rotation curve and of a map of our milky way. (experiment instructions)
- Chaos in the planetary system (Computational Physics, Christoph Schäfer room C10 A11, (Willy Kley room C10 A45), meeting place C9 G09)
In the classical N body problem the trajectories of N point masses in their common gravitational field are estimated. In this experiment, different numerical schemes for the solution of ordinary differential equations (ODEs) will be implemented and tested on the application to the integration of these trajectories. (web page of this experiment; poster)
- N-Body Simulations with REBOUND (Computational Physics, Christoph Schäfer room C10 A11, (Willy Kley room C10 A45), meeting place C9 G09)
In this part of the practical course, the students will use an existing N-Body software package to address several problems such as the stability of Saturn's rings and the Kirkwood gaps. (experiment instructions)
- Classical experiments of Astronomy: Pulsars and rotation of Mercury (Astronomy, N.N.)
This experiment is not offered in this semester. (experiment description (german) )
The posters of the experiments were presented during a labwork leader meeting held in Tübingen in September 2008.
Experiments in Nuclear Physics for students of Master Astro and Particle Physics:
- Nuclear Magnetic Resonance (David Blum, Tel. 73286, Büro D4 P44; Vincent Schipperges Tel. 77081, Büro D2 P07; Tobias Jammer Tel. 76283, Büro D2 A17; meeting place D3 O03)
Basic measurements with pulsed NMR using liquid and solid samples which demonstrate the fundamental principles behind magnetic resonance spectroscopy (MRS) and magnetic resonance imaging (MRI). (experiment instructions)
- Mößbauer Effect (Axel Müller, Tel. 73286, Büro D4 P44; Büsra Cebeci, Tel. 77081, Büro D2 P03; meeting place D2 P40)
The Mößbauer effect, or recoilless nuclear resonance fluorescence, allows to study tiny changes in nuclear energy levels. In this experiment the hyperfine splitting, isomeric shift and quadrupole splitting will be measured. (experiment instructions)
- Neutron Activation (Alexander Tietzsch, Tel. 73286, Büro D4 P44; Andreas Zschocke, Tel. 76288, Büro D4 P40; meeting place D2 P40)
Study of radioactive decay of different materials, which will be activated by a neutron source (like in nondestructive material testing) and analysis of correlation between decay and activation times. (experiment instructions)
Students of the specialized course in Astronomy and Astrophysics have to carry out 4 experiments of the section Astronomy and one experiment of the section Computational Physics. Within the section Astronomy the experiment Photometry and Spectroscopy is obligatory.
Students of Master Astro and Particle Physics have to carry out 2 experiments of the section Astronomy, one experiment of the section Computational Physics and 2 experiments of the section Nuclear Physics.
- It is expected that the experiment instructions are read and understood by the date of the experiment. This will be checked by an oral attestation prior to the beginning of the experiment. Some experiment instructions contain excercises and questions in the theoretical part, which should be solved and presented during this attestation. In case of unsufficient preparation the students may be excluded from the experiment.
- Successful participation in the basic module "Astronomy and Astrophysics" (study path Bachelor) or student of Master of Science Astro and Particle Physics.
- Basic knowledge in programming:
For the experiments carried out by Computational Physics it is expected, that the participants are able to write small programs by their own, e.g. in C or FORTRAN. Online tutorials are available on the web page Hints for the programming experiments. In case of questions or problems W. Kley resp. C. Schäfer will give some help.
- The analysis of the Astronomy experiments is done ususally with the programming and interpreter language IDL. The required steps are described in detail in the corresponding experiment instructions.
- For the experiment MCP detectors knowledge of Excel is helpful, but not really required.
- The experiment instructions of MCP detectors contains at the end a chapter with general Hints for writing a protocol. It is obligatory to read these hints prior to starting the labwork and to subsequently follow these hints!
- The programming experiments will take place in the computer room of the Theoretical Physics (CIP-Pool, Morgenstelle D2A38, login with the usual university account).