L1 TMSY Telescope focal tuning results Adam Mullavey, Chris Guido 31 Oct 2013 LIGO-G1400170.

Slides:



Advertisements
Similar presentations
Telescopes By Mr. King. Tube Stand Tube Stand eyepiece.
Advertisements

Optics and magnetic field calculation for the Hall D Tagger Guangliang Yang Glasgow University.
Light and Color for the Middle School By Greg Corder.
1 ATST Imager and Slit Viewer Optics Ming Liang. 2 Optical layout of the telescope, relay optics, beam reducer and imager. Optical Layouts.
M3 Instrument Design and Expected Performance Robert O. Green 12 May 2005.
Practical Optics Class Opti696D, Fall Laser Bar Code Scanner Chunyu Zhao.
Microscope Objective Parameters. What do the Numbers on the Objective Mean ?
Chapter 36 Image Formation EXAMPLES. Chapter 36 Image Formation: Examples.
Telescope Tear-Down Anatomy of a 114mm f/8 Newtonian Reflector.
Chapter 23 Mirrors and Lenses. Medical Physics General Physics Mirrors Sections 1–3.
Chapter 23 Mirrors and Lenses.
Announcements Exam 2 is scheduled for two weeks from today (April 2) but, due to all the missed days it will be pushed back one week to April 9 Homework:
Mirrors and Lenses: Mirrors reflect the light Lenses refract the light.
The Refraction of Light The speed of light is different in different materials. We define the index of refraction, n, of a material to be the ratio of.
FLAO Alignment Procedures G. Brusa, S. Esposito FLAO system external review, Florence, 30/31 March 2009.
LIGO-G9900XX-00-M adLIGO R&D1 AdLIGO Bench Testing of Proposed Quad Alignment & Gap Setting Hardware (Keyence)T Two SOS optics were used to represent.
Goal: To understand how mirrors and lenses work
Optics Can you believe what you see?. Optics Reflection: Light is retransmitted from or “bounces off” an object.
Status of IPBSM Improvement N. Terunuma, KEK 2012/July/13 ATF2 Weekly Meeting.
Camera Distance Tutorial Julie Morrow-Tesch, Jeff Dailey, Adam Lewis.
Chapter 30 Key Terms June 4 – June 10 Mr. Gaydos.
Ray Optics: Reflection and Refraction Rays Representation of the path that light follows Represent beams of light that are composed of millions.
Exploring Space Section 1 Radiation from Space Define: Electromagnetic spectrum Refracting telescope Reflecting telescope Observatory Radio telescope.
ILIAS WG1 meeting, 19/06/07 IB Faraday Isolator 1 IB in vacuum Faraday isolator E. Genin, S. Hebri, S. Hamdani, P. La Penna, J. Marque EGO.
$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.
PACS IIDR 01/02 Mar 2001 FPFPU Alignment1 D. Kampf KAYSER-THREDE.
13-3 and Notes Mirrors. Concave Mirror – An inwardly curved, mirrored surface that is a portion of a sphere and that converges incoming light. Concave.
FLAO system test plan in solar tower S. Esposito, G. Brusa, L. Busoni FLAO system external review, Florence, 30/31 March 2009.
How do I see color? Photochemical receptors receive the light (____ and _____) Rods-brightness cones-the color They release a ________ signal to the brain.
MICROSCOPE DESIGN. beam expander and objective Why do we need a beam expander? What facts about the laser do we need to know? How much expansion do we.
Oct 17, 2001SALT PFIS Preliminary Design Review1 Southern African Large Telescope Prime Focus Imaging Spectrograph Mechanical Mechanism Design Michael.
Plan in summer shutdown Magnet -SF1FF -Swap of QEA magnet - Multipole field of Final Doublet IP-BSM improvement.
Specifications for OMC telescope in AdVirgo R. Gouaty, E. Tournefier Estimation of carrier HOM power at the dark port Constraints on OMC waist and position.
1.Rationale and core concepts 2. Description of the activities 3. Target group 4. Materials 5. Setting of the class 6. Space and time 7. Didactics.
Images Formed by Lenses Ray Diagrams for Lenses Ray diagrams can be used to predict characteristics of images using 3 rays, just like for concave.
Current Balance MS&T Physics 2135, Lab E4.
LSC meeting, 25/05/07 Thermal lensing simulation 1 Faraday thermal lensing numerical simulations Slim Hamdani EGO LIGO-G Z.
Optics Refraction and Reflection. Law of Refraction How it works:
H2 TMS Y QPD Sled - As Built - Bram Slagmolen, Keita Kawabe, Matt Evans LIGO-T
Optimization of beam envelop at the injection point of PS Chenghui Yu Jan. 30, 2012.
MIRRORS. ACTUAL light path APPARENT light path OBJECTIMAGE: same size, equal distance behind normal 1. PLANE (FLAT) MIRROR VIEWER Law of Reflection: equal.
Ying Yi PhD Lab 5: Lenses 1 PHYS II HCC. Outline PHYS II HCC 2 Basic concepts: image, convex lens, concave lens, focal length Lab objectives.
M Manser WAVES : Optics (t riple science) By the end of this presentation you should be able to: Identify the differences between converging and diverging.
Lights, Mirrors, and Lenses Light is another type of wave that carries energy. A light ray is a narrow beam of light that travels in a straight line. Light.
17.1 Reflection and Refraction. Chapter 17 Objectives  Describe the functions of convex and concave lenses, a prism, and a flat mirror.  Describe how.
Design for a New Optical Table of the Shintake Monitor Takashi Yamanaka The University of Tokyo ATF2 weekly meeting 2007/9/26.
The reading is 7.38 mm. The reading is 7.72 mm.
Prism Pairs for Elliptical Beams
TMSY Telescope focal tuning results
Light.
Tolerances & Tuning of the ATF2 Final Focus Line
Chapter 32Light: Reflection and Refraction
Mirror Equations Lesson 4.
Answer the “4 big questions”.
Ordering Task – Object in Front of a Concave Mirror
Magnetic gap calculation
On the next five slides there is a “step-by-step solution”
Free-Response-Questions
Introduction to Microscopes!
Please see slide 2 for the caption of this figure.
Review calculation of Fresnel zones
3.1 “I Can draw circles, and identify and determine relationships among the radius, diameter, center, and circumference.”
DO NOW QUESTION What do you think when you hear the word “optics”?
Mirrors and Lenses.
Convex Mirrors.
3.1 “I Can draw circles, and identify and determine relationships among the radius, diameter, center, and circumference.”
Beam Tilt & TFC: Which z value for correction?
Physics Projects Color wheel Types of mirrors and uses
RHIC Spin Flipper M. Bai, T. Roser Collider Accelerator Department
Crab Crossing Named #1 common technical risk (p. 6 of the report)
Presentation transcript:

L1 TMSY Telescope focal tuning results Adam Mullavey, Chris Guido 31 Oct 2013 LIGO-G

Source Parameters (MM results) [EXTERNAL RESULTS] MinMaxMeanStd Dev Dim M≤x M≤y M≤r Wox mm 2Woy mm 2Wor mm 2Wex mm 2Wey mm 2Wer mm Zox m Zoy m Zor m Zrx mm Zry mm Zrr mm Divergencex mr Divergencey mr Divergencer mr Astigmatism(Zoy-Zox)/Zrr % Waist Asymmetry(2Woy/2Wox) Divergence Asymmetry Thetay/Thetax IR beam retro reflected using flipper mirror on periscope. The RED marked values are used for the model.

Tele Measurement - 1 (Single Lens) 1.IR beam into the Tele, retro-reflected by the 8” flat ETM, back to the MM. 2.The RED marked values are used in the model are return values. [EXTERNAL RESULTS] MinMaxMeanStd Dev Dim M≤x M≤y M≤r Wox mm 2Woy mm 2Wor mm 2Wex mm 2Wey mm 2Wer mm Zox m Zoy m Zor m Zrx mm Zry mm Zrr mm Divergencex mr Divergencey mr Divergencer mr Astigmatism(Zoy-Zox)/Zrr % Waist Asymmetry(2Woy/2Wox) Divergence Asymmetry Thetay/Thetax

Tele Measurement – 2 (Single Lens) 1.Same as ‘Tele Measurement – 1’, but with the ModeMaster rotated (roll) by 45 degrees, to sample the beam differently. 2.The RED marked values are used as the return values. [EXTERNAL RESULTS] MinMaxMeanStd Dev Dim M≤x M≤y M≤r Wox mm 2Woy mm 2Wor mm 2Wex mm 2Wey mm 2Wer mm Zox m Zoy m Zor m Zrx mm Zry mm Zrr mm Divergencex mr Divergencey mr Divergencer mr Astigmatism(Zoy-Zox)/Zrr % Waist Asymmetry(2Woy/2Wox) Divergence Asymmetry Thetay/Thetax

Telescope de-tuning Results (using TeleScan1 measurements) X-axisY-axis 1.Input into the TeleModel are the measured Source Parameters from the ModeMaster. 2.The GREEN markers are from the measured ModeMaster results from ‘Tele Measurement 1’ (they should be crossing the red calculated line). 3.The vertical lines indicate the tolerance.

Telescope de-tuning Results (using TeleScan2 measurements) X-axisY-axis 1.Input into the TeleModel are the measured Source Parameters from the ModeMaster. 2.The GREEN markers are from the measured ModeMaster results from ‘Tele Measurement 2’ (they should be crossing the red calculated line). 3.The vertical lines indicate the tolerance.