Mirror Alignment Using Dual Beam Laser

Slides:



Advertisements
Similar presentations
Built-In Test Software for Deformable Mirror High Voltage Drivers Built-In Test Software for Deformable Mirror High Voltage Drivers Jianwei Zhou Home Institution:
Advertisements

Scott Hamilton Bill Randolph University of Hawaii at Manoa W. M. Keck Observatory.
Measuring Turbulence in Domes Jeff Fines University of Hawai‘i, Manoa - BSEE Craig Nance W.M. Keck Observatory 25 July 2008.
1. SMA Project Description Background Design Construction Test Conclusion Acknowledgments 2.
1.  Background on AMiBA  Problems/Things to Consider  Solutions/introduce my project  Fabrication  Conclusion  Acknowledgments 2.
30-meter cabin refurbishment for a large Field Of View: status of on-going study S.Leclercq 28/04/2008.
Solar Orbiter EUV Spectrometer
Adaptive Optics Deformable Mirror Electronics Simulation Pearl Yamaguchi Subaru Telescope National Astronomical Observatory of Japan Mentor: Stephen Colley.
Active Control of Aberrations for the Large Synoptic Survey Telescope (LSST) Brice Cannon Lawrence Livermore National Laboratory Research Supervisor: Scot.
Walking the Beam §Often a laser can work but the beam is not parallel to the bore. §This results in serious losses and low output power. §If left unchecked.
CARMA. CARMA 225 GHz map with 0.9’’ beam (C-array) 1’’ is not good enough! BN? source I.
Darcy Bibb Oceanit Mentor: Tony Bartnicki Advisor: Curt Leonard Home Institution: Maui Community College Integration of a Small Telescope System for Space.
1 Built-In Test Software for Deformable Mirror High Voltage Drivers Jianwei Zhou Home Institution: University of Hawaii at Manoa CfAO Akaimai Intership.
Canada-France-Hawaii Telescope Observatory Automation Project: Audio and Video Management Project by: Amber Imai Mentors: Tom Vermeulen & Bill Cruise Advisor:
July 2015 doc.: IEEE /XXXXr0 July 2015
Setup of laser tracker on DX side NOTE: X axis along M1s centers, towards SX Z axis along M1-M2 centers, towards M2.
IRIS Telescope Camera Kimberly Bott Institute for Astronomy Mentor: Klaus Hodapp Home Institution: University of Hawaii at Hilo 2008 Center for Adaptive.
Jose Luis Sirvent Supervisor: Jonathan Emery Student Meeting 24 October 2011.
Concentration Measurements of Porphyrin Solutions using the Cavity Ring-Down and Integrated Cavity Output Spectroscopy Techniques Deirdre O’Leary PY4060.
Multiple Criteria Optimisation for Base Station Antenna Arrays in Mobile Communication Systems By Ioannis Chasiotis PhD Student Institute for Communications.
1 Mapping Maui’s Major Roads With Global Positioning System Devices Augustus Elias Center for Adaptive Optics Pacific Disaster Center Mentor: Pam Cowher.
Poster Presentations -preparing and presenting at your best- Malika Bell CfAO Summer, 2006.
Increasing Image Transfer Speed In MSAT Through Image Compression David Elies Akimeka, LLC Advisor: Steve Schweibinz Mentor: Rob Reed.
Characterization of Solar Cells Mary Liang Center for Adaptive Optics, Akamai Internship at Hnu Photonics Mentor: Dan O’Connell Home Institution: University.
Optical Tweezers Sarah Nichols March 17, Outline Motivations Operation Layout Successes and Difficulties Future Directions.
Creating a Parallel Program to Compute Statistical Information Victoria Sensano Maui Scientific Research Center Research Supervisor: Douglas Hope.
1 Automated Installation Windows Unattended Client PC Setup Vahid Ajimine W.M. Keck Observatory Mentor: Jason Ward Home institution: University of Hawaii.
1 Sun Tracking Stablility Through Imaging Tyson Seto-Mook Institute for Astronomy.
Laser Dye Performance A.Jaqueline Mena University of Hawai’i- Hilo W.M. Keck Observatory Mentor: Kenny Grace Advisor: Jason Chin Funding provided through.
Proprietary Wireless Network for the Digital Bus Kianiwai Spangler CFAO Akamai Internship Advisor: Alisa Manangan Supervisor: Cynthia Fox Akimeka, LLC.
Avian Influenza Modeling By: John Fujita Research Institution: Pacific Disaster Center Research Supervisor: Mike Napier Home Institution: University of.
Characterizing Lenslet Arrays for the Keck Adaptive Optics System Laboratory for Adaptive optics (LAO) UC Santa Cruz Name: Abubakarr Bah Home Institution:
Characterization and Upgrading of Adaptive Optics Demonstrator Joseph Curamen Maui Community College Mark Hoffman & Mark Ammons MCC & UCSC-CfAO.
The Akamai Observatory Short Course AOSC 07 Anticipated Core Team S. Anderson (Keck) : Hawaii Island Internship Program Coordinator D. Le Mignant.
By: Andrew Williams University of Rochester
CfAO Summer Internship Michelle Darrah Smithsonian SubMillimeter Array Supervisor: Alison Peck Dual Track Internship: Observing Assistant - learned how.
GSFC Scanning Holographic Receivers for Air and Space Geary Schwemmer Meeting of the Working Group on Space-based Lidar Winds Sedona, Arizona January 27.
Vacuum System Vibration Analysis on the Keck Telescopes Michael Cooney W.M. Keck Observatory.
1 Jennifer Takaki CfAO Akamai Observatory Internship Program Project Supervisor: Lucio Ramos Subaru Telescope, NAOJ Home Institution: Hawaii Community.
1 Measuring Deflection of the Telescope Mount Arlen Kam Gemini North Observatory Mentor: John White Supervisor: Neal Masuda.
Designing a Portable Data Acquisition Unit: Increasing Efficiency and Maximizing Productivity by Use of Standards Dustyn Iwamoto Home Institution: Honolulu.
Satellite Orbit Visualization Vladimir Ivanov Oceanit Project Supervisor: Frank Dachille Project Advisor: Dale Nahoolewa, Curt Leonard Home Institution:
Automating Astronomical Instrument Setup Eric J. Dela Rosa Hawaii Island Akamai Internship Canada France Hawaii Telescope Mentor : Gregory Barrick Advisor:
Shem Livai Institute for Astronomy Mentor: Colin Aspin Advisor: Bo Reipurth Home Institution: University of Hawaii at Manoa Funding provided through the.
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.
Optimizing the Throughput of an Optical System Lisa Phillips Textron Systems Mentor: Robert Nolan Advisor: Robert Lercari R&D Team: Tim Georges, Curtis.
Institute for Astronomy Herson Bagay Mentor : Garry Nitta Advisor : Jeff Kuhn.
Improved Imaging of Near Earth Objects Using Better Telescope Specifications Hazel Butler CfAO Akamai Internship Institute for Astronomy Advisors: Stuart.
Radiometric Calibration for the MAIA Laser Receiver Stacey R. Sueoka Mentor: Robert Nolan Supervisor: Don Ruffatto Textron Systems.
Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.
Built-In Test Software for Deformable Mirror High Voltage Drivers Built-In Test Software for Deformable Mirror High Voltage Drivers Jianwei Zhou Home Institution:
Thermodynamic Modeling o f Astronomical Infrared Instruments Francesc Andre Bertomeu Hartnell College Salinas, California Research Advisor: James Larkin.
Z Knight W.M. Keck Observatories Research Supervisor: Al Conrad Home Institution: University of Hawai'i at Hilo A Graphical User Interface for NIRC2 Asteroid.
Lawrence Livermore National Laboratory María Rosa Rivera Roque Research Supervisors: Shannon Ayers and Victor Sperry Research Advisor: Scot Olivier Educational.
CfAO Professional Development Workshop “Connecting Science Education Theory and Practice” Introduction Lisa Hunter Associate Director, Education.
Leader Interviews Name, PhD Title, Organization University This project is funded by the National Science Foundation (NSF) under award numbers ANT
Metrology of Prototype Nanolaminate Deformable Mirrors John Ruiz San Antonio College Lawrence Livermore National Laboratories Principle Investigator: Scot.
STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Possible layouts of Field Cameras.
Compressor Helium filled optional equivalent plane imaging laser beam dump hole in mirror for e-beam SSA and more.
A New WAVE of ENERGY Jasmine Yoshimoto Mentor: Ned Davis Maui Akamai Internship Program Internship site: Trex Enterprises August 4,
Generation of intense few-cycle pulses from the visible to the mid-IR Josh Nelson 1 Danny Todd 2 Adam Summers 3 Derrek Wilson 3 Dr. Carlos Trallero 3 1.
Beam Measurement Characterization and Optics Tolerance Analysis of a 900 GHz HEB receiver for the ASTE telescope Alvaro Gonzalez, K. Kaneko, Y. Uzawa.
From: Microtube Laser Forming for Precision Component Alignment
LCLS CXI Sample Chambers and Engineering Solutions
Development of a laser system for combining 3 laser beams
Why Do CPO Lead to Slow Light When the Laser
Figure 11-1.
Figure Overview.
Figure Overview.
Image Database Catalog
Presentation transcript:

Mirror Alignment Using Dual Beam Laser Vinya Agluba Smithsonian Astrophysical Observatory, Submillimeter Array Research Supervisor: Rob Christensen Home Institution: University of Hawaii - Manoa

Overview Antenna Optics Layout Importance of Mirror Alignment Aligning the Mirrors Conclusion

Antenna Optics Layout Figure 1

Antenna Optics Layout Figure 2

Importance of Mirror Alignment Achieve Maximum Efficiency Align Mirrors Reduce Losses -due to: beam truncation, distortion at focusing mirrors, and absorption and reflection at windows and mirrors 230GHz – 0.7-0.8 345GHz – 0.55-0.65 690GHz – 0.4

Aligning the Mirrors Figure 3

Aligning the Mirrors M5 M4 170mm Figure 4

Problem - Solution Figure 5

Problem - Solution Figure 6

XAWTV

First Trial

First Trial Elevation: 70° 20° 40°

DS9

Second Trial

Second Trial Elevation: 65° 85° 55° 75° 35° 15° 25° 45°

Second Trial

Targets 170mm

Conclusion Align mirrors using dual beam laser Use targets to ensure the 170mm height

Acknowledgments Rob Christensen & Ant Schinckel SMA Staff CfAO University of Hawaii - Manoa Funding provided through the Center for Adaptive Optics, a National Science Foundation Science and Technology Center (STC), AST-987683.