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Changes between Initial Version and Version 1 of OldPresentations2024


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Timestamp:
5 Mar 2025, 23:05:21 (4 days ago)
Author:
Vianak Naranjo
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  • OldPresentations2024

    v1 v1  
     1|| '''16.09.2024''' || '''Werner Laun''' || '''The METIS-cryostat'''[[BR]][[BR]]The new large ELT telescope is slowly growing on the Cerro Armazones in Chile. At the same time as the telescope is being built, the first generation of instruments is also being built. The MPIA is involved in 2 instruments, METIS and MICADO. For METIS, the MPIA has taken on two large work packages: the wavefront sensor and the imager. The design and construction of the cryostat, which is the subject here, are work packages of ETH Zurich. However, the MPIA was heavily involved in the initial concept and design. In the meantime, the first parts of the cryostat have arrived in Zurich and integration has begun.[[BR]][[BR]]This talk is intended to explain what a cryostat is and how this special cryostat for METIS is constructed. Colleagues who are not involved in instrumentation or science are also invited to attend.[[BR]][[BR]][[BR]]Presentation: German[[BR]][https://svn.mpia.de/trac/gulli/att/raw-attachment/wiki/WikiStart/AstroTechTalk_Metis_cryostat_16_09_2024.pdf Slides: English][[BR]]Questions: German, English ||
     2|| '''11.11.2024''' || '''Julian Stuermer (LSW)''' || '''CUBES'''[[BR]][[BR]]CUBES, the Cassegrain U-Band Efficient Spectrograph, brings a unique  capability to ESO’s Very Large Telescope:  an ultraviolet eye on the Universe to complement the Extremely Large  Telescope. CUBES aims to be the most efficient (> 40%) ground based  spectrograph in the UV with a spectral coverage of 300–405 nm. Two  resolution modes are offered: 20000 and 7000. [[BR]] [[BR]]The final design phase is currently being completed and it is expected  that manufacturing phase is starting early next year. [[BR]] [[BR]]The talk gives an overview of CUBES, with a focus of the technical  challenges in optics and mechanics. New grating technology enables high  efficiency in the UV, while an active flexure compensation supports the  spectral stability of the instrument.[[BR]][[BR]]Presentation: German[[BR]]Slides: English[[BR]]Questions: German, English ||
     3|| '''14.11.2024''' || '''Cécile Deprez (DLR Munich)''' || '''The Future of Satellite Navigation'''[[BR]][[BR]]At the German Aerospace Center (DLR), we are pioneering the  next generation of satellite-based positioning systems. Our research  focuses on integrating innovative technologies, including laser  communication links and optical clocks, into satellite payloads to  significantly enhance positioning accuracy for ground and space users.  [[BR]][[BR]]In this lecture, we will introduce the key concepts of satellite-based  positioning and present the solutions developed at DLR for the future of  global navigation.[[BR]][[BR]]Presentation: English[[BR]]Slides: English[[BR]]Questions: German, English ||