| APT |
Twin Automatic Photoelectric Telescopes "Wolfgang Amadeus"; robotic stellar photometry from southern Arizona |
| BMK10k |
A robotic wide-field telescope with a FOV of 50 square degrees to support the PLATO mission |
|
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3D radiation (magneto-) hydrodynamics code designed for the numerical simulation of stellar convection |
| iMAP |
Zeeman-Doppler Imaging code: Polarized radiative transfer based Stokes profile inversion for temperature and magnetic mapping. |
| GANS |
The night spectrograph for the German solar telescope GREGOR |
| GREGOR |
1.5-m optical solar telescope on Tenerife. The telescope will be able to resolve 70 km on the Sun. |
| LOFAR |
Low-Frequency Array: European antennae array for interferometry by super-computational treatment of the data stream. |
| NIRVANA |
Numerical code for 3D non-relativistic, compressible MHD with adaptive mesh refinement and self-gravity. |
| PEPSI |
Potsdam Echelle Polarimetric and Spectroscopic Instrument for the LBT |
| SOLARNET |
SOLARNET is a European network coordinating and promoting research infrastructures in the field of high-resolution solar physics. |
| STELLA |
Robotic telescopes for stellar activity. Instruments are an Echelle spectrograph and a wide-field imaging photometer. |
Programm Potsdam-Berlin-Kolloquium, 11.10.2019
