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Changes between Version 7 and Version 8 of AstroTechTalk


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Timestamp:
25 Aug 2014, 16:41:15 (10 years ago)
Author:
gaessler
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precision

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  • AstroTechTalk

    v7 v8  
    2626||'''Date''' ||'''Speaker''' ||'''Topic''' ||
    2727|| 12.09.2014 || Martin Kürster || ||
    28 || '''19.09.2014''' || '''Ralf-Rainer Rohloff''' || '''Exact metal optics over a large temperature range '''[[BR]] [[BR]]Since long, metal optics are an important part of astronomical instruments. Often [[BR]]diamond turned mirrors of aluminum (Al6061) are used. But it is difficult to polish [[BR]]aluminum. Therefore, the mirror is coated with Nickle Phosphor layer, which can [[BR]]be  polished  more  easily. This is very important  at shorter  wavelength. But  the [[BR]]mirrors  deform  with temperature changes  because of  the different coeffient of [[BR]]thermal expansion between aluminum and NiP. [[BR]][[BR]]Ralf-Rainer will tell us about a  collaboration between MPIA Heidelberg and IOF [[BR]]Jean, which  developed and  tested a new material to minimize the temperature [[BR]]related   deformation   of  such   mirrors. The  material   consists   of  an  aluminum [[BR]]silicate,  which  has  a coefficient of  thermal  expansion   close to  NiP. Thus,  the [[BR]]deformation could  be  reduced   drastically. But  now   the  work  just   started. Is it [[BR]]possible to built a mirror of this material? Does the material change with time? [[BR]]The best   answer  would  be  the  study  could  show  that such mirror  can be built [[BR]]and are stable over time! [[BR]][[BR]]Talk: German                                          [[BR]]Slides: English                              [[BR]]Questions: German, English ||
     28|| '''19.09.2014''' || '''Ralf-Rainer Rohloff''' || '''Precision metal optics over a large temperature range '''[[BR]] [[BR]]Since long, metal optics are an important part of astronomical instruments. Often [[BR]]diamond turned mirrors of aluminum (Al6061) are used. But it is difficult to polish [[BR]]aluminum. Therefore, the mirror is coated with Nickle Phosphor layer, which can [[BR]]be  polished  more  easily. This is very important  at shorter  wavelength. But  the [[BR]]mirrors  deform  with temperature changes  because of  the different coeffient of [[BR]]thermal expansion between aluminum and NiP. [[BR]][[BR]]Ralf-Rainer will tell us about a  collaboration between MPIA Heidelberg and IOF [[BR]]Jean, which  developed and  tested a new material to minimize the temperature [[BR]]related   deformation   of  such   mirrors. The  material   consists   of  an  aluminum [[BR]]silicate,  which  has  a coefficient of  thermal  expansion   close to  NiP. Thus,  the [[BR]]deformation could  be  reduced   drastically. But  now   the  work  just   started. Is it [[BR]]possible to built a mirror of this material? Does the material change with time? [[BR]]The best   answer  would  be  the  study  could  show  that such mirror  can be built [[BR]]and are stable over time! [[BR]][[BR]]Talk: German                                          [[BR]]Slides: English                              [[BR]]Questions: German, English ||
    2929|| 26.09.2014 || || ||
    3030|| 03.10.2014 ||-- ||Tag der deutschen Einheit ||