PDF-Adjustment (Collimation) of Newtonian Telescopes with the help of theL

Instruction Manual 2010 by Baader Planetarium GmbH Adjustment of Newtonian Telescopes with theLaserColli. Why are jammy rice pudding and foretelling the future incompatible? (Pages 8-9). C20 Problems:. With the emergence of quantum physics in the early C20, the . Uncertainty Principle. is born: one cannot, with absolute certainty, know both the velocity and position of a moving body.. 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. 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. Bien . positionner le miroir secondaire devant le . porte-oculaire. Normalement, ceci n'aurait pas à être fait plus d'une fois, soit la première fois que vous utilisez un nouveau télescope. Par le petit trou de l’oculaire de collimation vous devriez voir le miroir secondaire avec le miroir primaire qui s'y réfléchit. Le miroir secondaire devrait paraître centré et bien rond. . UA9 experiment. Emelie Nilsson. Chalmers University of Technology, Sweden. Supervisor: Dr. Walter . Scandale. . OUTLINE. 1/9/11. Student's coffee session. Crystal collimation- the theory. UA9 experiment in SPS. e. r . N. o. n. -. N. e. w. t. o. n. i. a. n. F. l. u. i. d. s. By: . Honzoda. . Abidjanova. TABLE OF CONTENTS. OOBLECK. KETCHUP. SILLY PUTTY. FLUBBER . CARAMEL . CUSTARD. BIBLIOGRAPHY. THE END. WHAT IS OOBLECK ?. reach. R. . . Bruce, . R. Assmann,. M. . Cauchi. , D. . Deboy. , L. . Lari, . S. . . Redaelli, A. . Rossi, . B. . Salvachua, G. . Valentino. Acknowledgements. :. W. . Herr, . M. Lamont, R. . de . Maria, . Zhirong . Huang. March 6, 2012. FLS2012 Workshop, Jefferson Lab. Outline. Introduction. Seeding and TW. Attosecond. pulses. Better beams. SASE wavelength range: . 25 – 1.2 . Å. Photon energy range: . . 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.