STC "VOSKHOD", PROJECT "SPECTR-UV", 27-30 JUNE 2006 Next slide Next slide Previous slide Possible layouts of Field Cameras.

Slides:



Advertisements
Similar presentations
Ray optics. Every point on a luminous or illuminated surface produces light rays in all available directions.
Advertisements

CMSC 2006 Orlando Active Alignment System for the LSST William J. Gressler LSST Project National Optical Astronomy Observatory (NOAO) Scott Sandwith New.
1 ATST Imager and Slit Viewer Optics Ming Liang. 2 Optical layout of the telescope, relay optics, beam reducer and imager. Optical Layouts.
TPC meeting, CERN, 7-8 October 2003Børge Svane Nielsen, NBI1 Status of laser system TPC meeting, CERN, 7-8 October 2003 Børge Svane Nielsen, Niels Lindegaard,
Basic Illuminating Light Paths and Proper Microscope Alignment E. D. Salmon University of North Carolina at Chapel Hill.
PACS IIDR 01/02 Mar 2001 Baffle and Straylight1 D. Kampf KAYSER-THREDE.
SWD 2005, Taormina, Jun,19-26 An EUV Imaging Detector of Space Solar Telescope Qian Song, Binxun Ye, Zhaowang Zhao National Astronomical Observatories,
Telescope Tear-Down Anatomy of a 114mm f/8 Newtonian Reflector.
FLAO Alignment Procedures G. Brusa, S. Esposito FLAO system external review, Florence, 30/31 March 2009.
Using Nodal Aberration Theory to Understand the Aberration Fields of Multiple Unobscured TMA Telescopes Kevin P. Thompson/ORA Tobias Schmid/CREOL Kyle.
NGAO Instrumentation Overview September 2008 Updated Sean Adkins.
The Research School of Astronomy and Astrophysics of the Australian National University at Mt Stromlo Observatory is developing a wide-field Cassegrain.
Twenty years ago IRAS gave us what is still our best view of the mid  infrared sky.
NGAO Alignment Plan See KAON 719 P. Wizinowich. 2 Introduction KAON 719 is intended to define & describe the alignments that will need to be performed.
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,
NGAO NGS WFS design review Caltech Optical Observatories 31 st March 2010.
Performance analysis of NGAO NGSWFS with and without the IF dichroic Caltech Optical Observatories 6 th April, 2010.
Spherical Mirrors - Starter
Status of IPBSM Improvement N. Terunuma, KEK 2012/July/13 ATF2 Weekly Meeting.
Setup of laser tracker on DX side NOTE: X axis along M1s centers, towards SX Z axis along M1-M2 centers, towards M2.
ASTRI SST-2M The Prototype monolithic 1.8 m
Integration and Alignment of Optical Subsystem Roy W. Esplin Dave McLain.
The Universe in the Infrared What is the Spitzer Space Telescope, and how does it work? Funded by NASA’s Spitzer Science Center Images courtesy NASA/JPL.
PACS IHDR 12/13 Nov 2003 PACS FPU Optics: Concept and Alignment R. Graue, D. Kampf Kayser-Threde.
Mirrors Plane and Spherical. Plane Mirrors Flat mirrors. Which type of image? Virtual We perceive the image at point I where the ray extensions intersect.
SALT Technology Development Lisa Crause India-South Africa Astronomy Workshop – SAAO 6 August 2012.
Engineering: NAHUAL Ireland Acquisition Camera, Focal Plane Mechanisms and Layout Tully Peacocke, National University of Ireland Maynooth Carlos del Burgo,
The Mid-Infrared Instrument (MIRI) Medium Resolution Spectrometer for JWST Martyn Wells MIRI EC & UKATC.
When light travels from an object to your eye, you see the object. How do you use light to see? 14.1 Mirrors When no light is available to reflect off.
PACS IIDR 01/02 Mar 2001 FPFPU Alignment1 D. Kampf KAYSER-THREDE.
1 of 28 A design study of a Cryogenic High Accurate Derotator.
Integral Field Spectrograph Eric PRIETO CNRS,INSU,France,Project Manager 11 November 2003.
Precision Layout Unit 21.
1 Jim Thomas - LBL New Pad Plane Design Proposal & Specifications Jim Thomas, John Hammond, Bob Scheetz, Jon Wirth, etc., etc., and a cast of thousands.
ZTF Optics Design P. Jelinsky ZTF Technical Meeting 1.
LIGO-G0200XX-00-M LIGO Scientific Collaboration1 First Results from the Mesa Beam Profile Cavity Prototype Marco Tarallo 26 July 2005 Caltech – LIGO Laboratory.
The Active Optics System S. Thomas and the AO team.
LSC August G Z Gingin High Optical Power Test Facility (AIGO) 1 High Optical Power Test Facility - Status First lock, auto-alignment and.
Delta II 7925H - 10L Baseline workup Launch Vehicle TheirsOurs Delta II 7925H Launch Vehicle 10L Composite Fairing 10L Stretch Composite Payload Fairing.
Oct 17, 2001SALT PFIS Preliminary Design Review1 Southern African Large Telescope Prime Focus Imaging Spectrograph Mechanical Mechanism Design Michael.
Low Polarization Optical System Design Anna-Britt Mahler Polarization Laboratory Group College of Optical Sciences.
Survey, Alignment and Metrology Fiducials Requirements Fabien Rey ESS Survey, Alignment and Metrology Group ACCELERATOR TECHNICAL BOARD 23/09/2015.
Mechanical design meeting, IAG, Calibration Unit mechanical design Svend M. Bauer Andreas Kelz, Emil Popow, Martin M. Roth.
ZTF Optics Design ZTF Technical Meeting 1.
Wide field telescope using spherical mirrors Jim Burge and Roger Angel University of Arizona Tucson, AZ Jim
Page 1HMI/AIA Science Meeting – February 13, 2006 HMI Instrument Status HM/AIA Science Meeting February 13, 2006 Barbara Fischer HMI Deputy Program Manager.
Wes Ousley June 28, 2001 SuperNova/ Acceleration Probe (SNAP) Thermal.
The Field Camera Unit Results from technical meeting S. Scuderi INAF – Catania.
J. H. Burgea,b, W. Davisona, H. M. Martina, C. Zhaob
Compressor Helium filled optional equivalent plane imaging laser beam dump hole in mirror for e-beam SSA and more.
PACS IIDR 01/02 Mar 2001 Optical System Design1 N. Geis MPE.
Seminar Autocollimator On
Astronomical Spectroscopic Techniques. Contents 1.Optics (1): Stops, Pupils, Field Optics and Cameras 2.Basic Electromagnetics –Math –Maxwell's equations.
Page 1 GSI, Hydraulic Actuators for PANDA Target Spectrometer Jost Lühning, GSI Darmstadt Functional Specifications for moving the TS: Two synchronous.
Update on electron spectrometer measurements Introduction Setup, measurements carried out Some raw images Results and conclusions L. Deacon, M. Wing (UCL)
Date of download: 9/17/2016 Copyright © 2016 SPIE. All rights reserved. Sampling points for (a) Fe nm and (b) Ca nm lines in the case of standard.
Integral Field Spectrograph Opto-mechanical concepts PIERRE KARST, JEAN-LUC GIMENEZ CPPM(CNRS),FRANCE.
More Zemax screenshots of the optical setup of the NIKA prototype installed since June 2012 at its final permanent position at the 30m telescope. S. Leclercq,
BWS Design meeting Jose Luis Sirvent PhD. Student XX/03/2014
Anatomy & Physiology of a Camera
Scott Wakely University of Vengeance
Interference Requirements
An IFU slicer spectrometer for SNAP
Intra-pixel Sensitivity Testing Preliminary Design Review
C2PU TELESCOPES Version 02, 28/08/2016 Jean-Pierre Rivet CNRS, OCA,
Progress on 1.8m Telescope with 127-element Adaptive Optics at IOE
Optical Design For a 32 Inch, All-Spherical Relay Cassegrain Telescope
Henry Heetderks Space Sciences Laboratory, UCB
C2PU TELESCOPES Version 02, 28/08/2016 Jean-Pierre Rivet CNRS, OCA,
Optics Alan Title, HMI-LMSAL Lead,
Presentation transcript:

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Possible layouts of Field Cameras

Next slide Next slide Previous slide Previous slide Configuration of Field Cameras ( )

The Fields of View Configuration for Field Cameras built on the detectors with 26 mm useful diameter (development of the Science Technology Center "Voskhod", ) Next slide Next slide Previous slide Previous slide

Instruments Configuration of the Field Cameras Unit built on the detectors with 26 mm useful diameter (development of the Science Technology Center "Voskhod", ) Next slide Next slide Previous slide Previous slide Overall dimensions of the Field Cameras Unit (assessment): - height – 230 мм - diameter (over the boundary points of the structure) – 650 mm

Next slide Next slide Previous slide Previous slide

Mounting Places for Field Cameras on the Force Body of the Field Cameras Unit (development of the Science Technology Center "Voskhod", ) Mounting Place of Short-focus Field Camera Mounting Place of Long-focus Field Camera Next slide Next slide Previous slide Previous slide

Field camera layout (variant) Next slide Next slide Previous slide Previous slide

Ray Path in the Long-focus Field Camera (variant) From the Secondary Mirror of the telescope Folding Spherical Mirror (Long-focus Mode) Next slide Next slide Previous slide Previous slide

Next slide Next slide Previous slide Previous slide Field Camera Unit Assembly and Alignment Philosophy  Field Cameras are aligned independently  Light-splitting Unit is mounted to the force body of the Field Camera Unit (as variant)  Field Cameras are mounted to the force body of the Field Camera Unit and aligned relatively the Light-splitting unit  Field Camera Unit is mounted to the Optical Bench of the Primary Mirror Unit and aligned relatively the telescope objective as a whole

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006  for the Central Field Camera placed in the Focal Plane of the telescope T-170M:  for the Central Field Camera placed offset to the optical axis of the telescope: variant  Cenrtal Field Camera  2 offset Sort-focus Filed Cameras  2 offset Long-focus Filed Cameras  3 Guide sensors + 1 place for the fourth sensor variant  Cenrtal Field Camera (with beam transfer)  3 offset Sort-focus Filed Cameras  3 Guide sensors Next slide Next slide Previous slide Previous slide Variants developed in 2006 for two Spectrometers and Central Field Camera

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 (See information on MCP (See information on MCP (Micro Channel Plate)) (Micro Channel Plate)) Next slide Next slide Previous slide Previous slide

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Previous slide

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 top viewbottom view Next slide Next slide Previous slide Previous slide  Cenrtal Field Camera  2 offset Sort-focus Filed Cameras  2 offset Long-focus Filed Cameras  3 Guide sensors + 1 place for the fourth sensor

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Spreadsheet for variant of Field Cameras layout for the Central Field Camera placed in the Focal Plane of the telescope T-170M Next slide Next slide Previous slide Previous slide

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Previous slide

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Previous slide

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Previous slide top viewbottom view  Cenrtal Field Camera (with beam transfer)  3 offset Sort-focus Filed Cameras  3 Guide sensors

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Previous slide Previous slide Spreadsheet for variant of Field Cameras layout for the Central Field Camera placed offset to the optical axis of the telescope

STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Return to variants-2006 Return to variants-2006 description