1 Progress in understanding flatness measurements Tom Diehl November 24, 2005 Draft as of 11/24/05.

Slides:



Advertisements
Similar presentations
PREX main detector Piotr Decowski Aimee Shore Smith College Piotr Decowski Aimee Shore Smith College Kumar Krishna Jon Wexler Patrick Rogan Vireak Yim.
Advertisements

DYnamical and Microphysical Evolution of Convective Storms Thorwald Stein, Robin Hogan, John Nicol DYMECS.
Laser Speckle Extensometer ME 53
A vertical-flexure CCD module Bruce C. Bigelow University of Michigan Department of Physics 10/7/04.
Understanding and Comparing Confocal Scanning Lasers to Optical Coherence Tomography for Optic Nerve Head Analysis (ONH) A presentation courtesy of Zeiss.
Optical Astronomy Imaging Chain: Telescopes & CCDs.
And a head sensor on a sun tracker What is PANDORA? Pandora is a small spectrometer system, which we have been developing since It consists of …
Range Imaging and Pose Estimation of Non-Cooperative Targets using Structured Light Dr Frank Pipitone, Head, Sensor Based Systems Group Navy Center for.
Pore Detection in Small Diameter Bores The University of Michigan, Ann Arbor NSF Engineering Research Center for Reconfigurable Manufacturing Systems.
Overview of XMM-Newton XMM-Newton carries three, co-aligned, densely-nested, grazing incidence telescopes, collectively providing unparalleled effective.
MSU/CSE Fall Computer Vision: Imaging Devices Summary of several common imaging devices covered ( Chapter 2 of Shapiro and Stockman)
REU Capillary Project Report, August 13, 2010 CHESS & LEPP REU Capillary Project Report August 13, 2010 Tia Plautz, Mark Pfeifer, Tom Szebenyi, Gavrielle.
Abstract At the Thomas Jefferson National Accelerator Facility in Newport News, Virginia, a team of nuclear physicists has come up with a way to probe.
Optical Alignment with Computer Generated Holograms
Spectrophotometer Jan 28, 2002 Deryck Hong Suryadi Gunawan.
Use of a commercial laser tracker for optical alignment James H. Burge, Peng Su, Chunyu Zhao, Tom Zobrist College of Optical Sciences Steward Observatory.
Wide-field, triple spectrograph with R=5000 for a fast 22 m telescope Roger Angel, Steward Observatory 1 st draft, December 4, 2002 Summary This wide-field,
The AMS-02 detector is based on a large acceptance (~0.5 m²sr) and high sensitivity spectrometer composed by a super-conducting magnet (0.8 T), cooled.
GE Energy Silicon Wafer Measurement System Team 10 Olin Biddy Scott Johnson Chetwyn Jones Rob McCoy Tim Weber.
Science Specification Table 12 keV keV for neutral particles 40.5 cm 2 image plane Electronic Noise 3 keV FWHM Proton Dead Layer
Image formation & Geometrical Transforms Francisco Gómez J MMS U. Central y UJTL.
Optical Design for an Infrared Multi-Object Spectrometer R. Winsor, J.W. MacKenty, M. Stiavelli Space Telescope Science Institute M. Greenhouse, E. Mentzell,
ISAT 303-Lab3-1  Measurement of Condition: Lab #3 (2005):  List of parameters of condition: –Linear distance, angular displacement, vibration, displacement,
NA62 Gigatracker Working Group Meeting 2 February 2010 Massimiliano Fiorini CERN.
Light, Mirrors, and Lenses O 4.2 Reflection and Mirrors.
Fiber-Optic Accelerometer Using Wavefront-Splitting Interferometry Hsien-Chi Yeh & Shulian Zhang July 14, 2006.
Notre Dame extended Research Community NANOWeek: The Power of Microscopes Optics Visible light Optical microscopes and telescopes Scanning electron microscope.
Science Impact of Sensor Effects or How well do we need to understand our CCDs? Tony Tyson.
IPD Technical Conference February 19 th 2008 Friction Roller Identification Jack Weatherford Hermitage Automation & Controls.
14 October Observational Astronomy SPECTROSCOPY and spectrometers Kitchin, pp
Understanding typical users for this instrument Graduate studentGraduate student –not an X-ray expert but wants to make a spatially resolved measurement;
Analysis of Metrology Data from First Two Small Disks Stephen Pate 5/11/111.
NORDFORSK Summer School, La Palma, June-July 2006 NOT: Telescope and Instrumentation Michal I. Andersen & Heidi Korhonen Astrophysikalisches Institut Potsdam.
The Hobby-Eberly Telescope Mirror Alignment Recovery System Marsha Wolf Graduate Student UT Astronomy Department.
Top surface of B3L Top surface of B3L B3L12 Tried to blow off, but couldn’t Insde of tube. B3L15 The dot at the middle.
September 16, 2008LSST Camera F2F1 Camera Calibration Optical Configurations and Calculations Keith Bechtol Andy Scacco Allesandro Sonnenfeld.
Silicon /pcb assembly R Thompson, J Freestone LAL 3 June 08.
Freiburg 7/07/20001 laser beam lens CCD (long arm) screen + grid CCD (short arm) glass plates at  45° STAMP : Saclay Telescope for the Alignment of Many.
BARREL ALIGNMENT PLATFORM POSITIONING Goal: Positioning of the platforms at their nominal position on the MDT chambers (No position measurement in a database).
Assessing Single Crystal Diamond Quality
Improvement of Infrared Lights Sensitivity on PZT EMITER Daisuke Takamuro, Hidekuni Takao, Kazuaki Sawada and Makoto Ishida.
W. Wester, Fermilab DES Callibration Meeting Jan 18, DECal scans update The DECal flat field system is capable of generating system response maps.
Notre Dame extended Research Community NANOWeek: The Power of Microscopes Optics Visible light Optical microscopes and telescopes Scanning electron microscope.
Current Status of Pepperpot Emittance Measurement System Simon Jolly Imperial College FETS Meeting, 22/02/06.
FETS Pepperpot Simon Jolly 10 th February The Pepperpot Beam segmented by intercepting screen with regular array of holes. Beamlets drift short.
Dimensioning the focal plane (RSC centric version) C. Bebek 9 July 2003 Revised 14 July 2003.
LCFI Mechanical room LCFI facilities –Cold survey cryostat and LASS, currently being upgraded –Cold gas test rig –Glue robot All housed in Lab 9 –Temperature.
Lesson 7 Development of cones with a cut surface.
Philtec Positioning Device D63 SENSORS. DC Spark System D63 Sensor Context: – Philtec was contacted to ask for the possibility of installing a new positioning.
다양한 창문을 통한 우주 내용 왜 다양한 창문 ? 왜 다양한 창문 ? 대기의 영향 대기의 영향 망원경의 성능 망원경의 성능 관측에서 얻는 정보 관측에서 얻는 정보 중요 망원경들 중요 망원경들 차세대 망원경들 차세대 망원경들.
Cloudland Instruments Hawkeye Mechanical Design Snapshot Compiled April 8th, 2016.
Date of download: 6/3/2016 Copyright © 2016 SPIE. All rights reserved. Laser-beam path through the engine’s cylinder head for ignition-window testing (schematic).
Outline Sample preparation Instrument setting Data acquisition Imaging software Spring 2009AFM Lab.
Microscope Parts.. Parts of the Microscope You should know all the parts of the microscope indicated:
NCSLI 2007 In House Capability of an Optical CMM Calibration for any Company Shawn Mason Boston Scientific.
SCANNING LIDAR FLUOROSENSOR FOR REMOTE DIAGNOSTIC OF SURFACES Luisa Caneve F. Colao, R. Fantoni, L. Fiorani, A. Palucci ENEA - UTAPRAD Technical Unit Development.
H. MAINAUD DURAND on behalf of the CLIC active pre-alignment team oWPS versus cWPS OUTLINE Introduction oWPS cWPS Results of inter-comparison tests
Optical System Review. Lens concept selections Solving the optical parameters (Magnification) (Focal length), Where, S’ is the distance from the lens.
Introduction to Precision Metrology
Thin Diamond Radiator Fabrication for the GlueX Experiment
AAFS 2004 Dallas Zeno Geradts
CLAS12 – RICH RICH - TECHNICAL PARAMETERS PARAMETER DESIGN VALUE
4x8 Mosaic Camera Development
Metrology and Trimming of CCD Detector Height
Probe-card Healthness Check-up
MultiView 400™ Product Presentation Nanonics MultiView 400™
FocalSpec Ltd High precision 3D and tomographic imaging sensors and systems Unique world wide patented Lateral Chromatic Imaging (LCI) technology Laboratory.
Intra-pixel Sensitivity Testing Preliminary Design Review
Automated Spotsize Measurements
Microscopy.
Presentation transcript:

1 Progress in understanding flatness measurements Tom Diehl November 24, 2005 Draft as of 11/24/05

2 Micro-Epsilon Opto-NCDT 2400 We need to control the flatness of the focal plane. We need to control the flatness of the focal plane. We need to measure components without touching their surfaces. We need to measure components without touching their surfaces. Using a DEMO version Jim Fast determined that this device could measure the distance to the surface of a CCD mounted in the test dewar through the dewar’s quartz window. Using a DEMO version Jim Fast determined that this device could measure the distance to the surface of a CCD mounted in the test dewar through the dewar’s quartz window. 100 micron spot diameter 100 micron spot diameter 24 mm measurement range at 222 mm distance 24 mm measurement range at 222 mm distance ~1 micron resolution ~1 micron resolution

3 Power Supply Polychromatic Light Source DSP Spectrometer Sensor On X-Y Stager DigitalOutput To Labview Controls Fiber Optic Cable   CCD Micro-Epsilon Opto-NCDT 2400

4 The Machinery Labview controls Labview controls X and Y dimension Stages w/ ~1 micron precision On the scale of our devices Micro-epsilonimager Sample

5 Silicon on a pedestal Example of a ¼ mm x ¼ mm scan of a part with very reflective surface. Non-flat surface features are evident. Example of a ¼ mm x ¼ mm scan of a part with very reflective surface. Non-flat surface features are evident.

6 Silicon Piece 6 cm x 3 cm Glued to aluminum nitride substrate Glued to aluminum nitride substrate Taped to a piece of unistrut. The device overlaps the unistrut by ~ 1 cm on each side. Taped to a piece of unistrut. The device overlaps the unistrut by ~ 1 cm on each side. Surface has observable grind marks from a thinning process. Surface has observable grind marks from a thinning process.

7 2 Images of Same Device ½ mm x ½ mm grid ½ mm x ½ mm grid Offset by 0.1 mm in Offset by 0.1 mm in Y direction illustrates the problem. One can see the warp in One can see the warp in the surface but only that general feature matches. Individual points do not.

8 Systematic Uncertainty The measurements of a point on the surface hold within about 1 micron. The measurements of a point on the surface hold within about 1 micron. If I move off and move back on the measurement repeats. If I move off and move back on the measurement repeats. If I move by off by 1/10 mm, the measurement is more different than what I think is the height of the typical surface feature. Spurious reflections from the grind marks trick the system? If I move by off by 1/10 mm, the measurement is more different than what I think is the height of the typical surface feature. Spurious reflections from the grind marks trick the system? A systematic unc’y is determined from 2 measurements offset by 1/10 mm. A systematic unc’y is determined from 2 measurements offset by 1/10 mm. deltaZ=delta(Z a -Z b )/sqrt(2)~15 micronsdeltaZ=delta(Z a -Z b )/sqrt(2)~15 microns

9 “Greg’s Device” 6 cm x 3 cm Average the measurements in ½ cm x ½ cm array. The total uncertainty on mean in each of the 72 regions is ~ 1 micron. Average the measurements in ½ cm x ½ cm array. The total uncertainty on mean in each of the 72 regions is ~ 1 micron. 13/72 regions gt 10 microns

10 The Plan A few more improvements to the Labview program A few more improvements to the Labview program Automation is pretty good.Automation is pretty good. Surface feature identification and concentration is nearly doneSurface feature identification and concentration is nearly done Bring into the CCD testing Lab Bring into the CCD testing Lab operate through a windowoperate through a window Incorporate results into the DES CCD database Incorporate results into the DES CCD database Develop a flatness grade for each CCDDevelop a flatness grade for each CCD Develop a way to test the DES Focal plane assembly Develop a way to test the DES Focal plane assembly