PDF-Adjustment (Collimation) of Newtonian Telescopes with the help of theL
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Instruction Manual 2010 by Baader Planetarium GmbH Adjustment of Newtonian Telescopes with theLaserColli
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Adjustment (Collimation) of Newtonian Telescopes with the help of theL: Transcript
Instruction Manual 2010 by Baader Planetarium GmbH Adjustment of Newtonian Telescopes with theLaserColli. Bruce C. Brown. Main Injector Department. 29 July 2015. Meeting Outline. BCBrown. (5 min) Introduction and Issues . Igor . Tropin. (15 min) Status MARS/MAD-X Tools. Essential Questions- You should be able to answer these questions by the end of the PowerPoint.. What is the purpose of a telescope?. How do refracting telescopes work?. How do reflecting telescopes work?. Telescopes. Key Concepts. What are the regions of the electromagnetic spectrum?. What are telescopes and how do they work?. Where are most large telescopes located?. Telescopes - Key Terms. Telescope. Telescopes were first invented around the year 1600. . Galileo . Galilei was an early astronomer who first used telescopes to view objects in our solar system. . He . made many important discoveries including: the moon was covered in mountains and Jupiter had 4 large moons.. Jon Holtzman. NMSU Astronomy. Telescopes are light buckets: bigger buckets collect more light, and faint (far away) objects don’t produce much light!. Why build bigger telescopes?. In principle, bigger telescopes make sharper images:. Optical Telescopes. Ground based and on satellites. Observations are recorded using a camera instead of the human eye most times. . This is so we can separate colors into light and using times to study changes over time.. The most important property of a telescope? . No, it’s not it’s “power” or magnifying ability, it is……. Its . Light Gathering . power! So, . t. he diameter of the mirror or lens is THE most important property. Types of Telescopes. A telescope collects light over a large area and focuses it in a . small area where it can be viewed with an eye or a camera. This can be done in 2 ways:. Refracting Telescopes. R. Assmann. 25.3.2010. Joint Meeting SPS Upgrade Study Group and SPS Task Force. Introduction. This is a brain-storming talk.. No detailed technical work done but enough to . explore and discuss a collimation option for SPS. An RVAS Meeting Program. By Frank Baratta. March 20, 2017. Horsehead Nebula: Public domain image at PixaBay.com. © F. Baratta, 2017; Graphics and images © F. Baratta, 2017, except as noted . . . . bad collimation is the number one killer of telescopes, world wide . . .. Refraction is the _____________ of light as it passes through glass.. II. Reflection: . Reflection occurs when light _____________ off of a mirror.. F. f. I. Refraction: . Refraction is the ___. bending. History. In 1773 Herschel invented a large . reflecting . telescope and discovered Uranus. This was the first “new” planet.. In late 1800’s . Kuiper. found methane gas in Saturn’s moon with the largest . . Size does matter. The bigger, the better. 2. Resolve detail. 3. Magnification. Only important for solar system objects. Refracting Telescopes. Cheap. Good for bright objects. Basic design. Reflecting Telescopes. TeV. R. Bruce, . A. Mereghetti. , S. Redaelli, B. . Salvachua. rMPP. . Meeting, CERN, . 26. th. Oct . 2015. DS . downstream of . IR7. :. Affected by . leakage. from . betatron. . collimation. system (single diffractive events);.
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