PPT-TMSY Telescope focal tuning results

Bram Matt and Keita 20 Oct 2011 LIGOG1101254 TMS Telescope Folded offaxis parabolic telescope Primary 9 diameter 2286 mm Front telescope aperture 85 Secondary 15 diameter 381 mm. 49 BelAir 103 Levis Qc Canada G6V 6K9 mrueltopcontrolcom Keywords Process Control Optimization Oscilla tion Model PID Control Closed L oop Open Loop Stiction Backlash Non linearity Pseudorandombinary Sequence Generalized Binary Noise ABSTRACT Tradit Introduction to Physics II. . Class 7 – . Outline:. Ch. . 24. Lenses in Combination . The . Camera . Vision . Microscopes. , Telescopes . Resolution . of Optical Instruments. Lenses in Combination. Ritva. A. Keski-Kuha, Charles W. Bowers, Manuel A. Quijada. NASA/Goddard Space Flight Center. James B. Heaney, SGT Inc. Greenbelt. Benjamin Gallagher, Ball. . Aerospace & Technologies Corp. Andrew McKay Northrop Grumman Aerospace Systems. Physics 2415 Lecture 34. Michael Fowler, . UVa. Today’s Topics. The . lensmaker’s. formula. Magnifying power. Lens combinations: ray tracing, telescopes.. Refraction at a Spherical Surface. Rays close to the axis (“paraxial”) will focus to an image inside the glass:. structure . following the consolidation . of . the requirements. Enrico . Giro – . INAF OAPD. for the ASTRI Collaboration & the CTA . Consortium. Universidade. . de . São. . Paulo. Instituto. Astronomical Instruments. The Formation of Images. Suppose we want to apply some of the properties of light discussed in the last session?. Recall the refraction of light through a prism?. Forming Images. 1. Outline. Issues and liens on JDEM-. Ω. Pros and cons for unobstructed aperture telescope. Review of trade space among various unobscured 3-mirror anastigmat (. uTMA. ) options that we have explored. So, if you are not sure, do your best to guess.. Please bring pencil(s) so that you can fill out. the scantrons.. No other accessories (calculators, cell phones, …) are allowed.. Important: Anything in the posted slides that I did not cover in class could be on the exam.. RED. for Web Traffic. Mikkel Christiansen, Kevin Jeffay,. David Ott, Donelson Smith. UNC, Chapel Hill. SIGCOMM 2000, Stockholm. subsequently. IEEE/ACM Transactions on Networking. Vol. 9 ,  No. 3  (June 2001) pp 249 – 264.. The Tuning Process. Benefits of Tuning. Why Tuning is Different. What is Tuning?. A collaborative, faculty-driven . process that . “harmonizes” curricula around defining what a . student should know and be able to do in a chosen . Diffraction of Light. Newton pointed . out in his 1704 book . Opticks. , that "Light is never known to follow crooked passages nor to bend into the shadow". . This concept is consistent with the particle theory, which proposes that light particles must always travel in straight lines.. Ninth Edition. Neil F. Comins • William J. Kaufmann III. CHAPTER 3. Light and Telescopes. WHAT DO YOU THINK?. What is light? . What type of electromagnetic radiation is most dangerous to life?. What is the main purpose of a telescope? . Telescope Specs.. Aperture X f-ratio = f or . fl. 98 x 6.3 = 617 . Eyepiece Focal Length in mm. AFOV - Apparent Field of View. Note: Not present on all Eyepieces. Eyepiece Formulas. Magnification = Telescope focal length ÷ Eyepiece focal length. Adam Mullavey, . Chris Guido. 31 . Oct. . 2013. LIGO-. G1400170. Source Parameters (MM results). [EXTERNAL RESULTS]. . Min. . Max. . Mean. . Std. . Dev Dim....