990901EIS_RR_HV.1 Heritage and Validation Approach Dr. Clarence M. Korendyke EIS US Project Scientist Naval Research Laboratory 202-767-3144

Slides:



Advertisements
Similar presentations
EIS Design Optimization Criteria Overall Length < 3 meters Overall Width < 0.5m Telescope Mirror Diameter 150mm Plate scale 1 arc-sec/pixel spatial –13.5.
Advertisements

M3 Instrument Design and Expected Performance Robert O. Green 12 May 2005.
Spectral Resolution and Spectrometers
990901EIS_Opt.1 The Instrument: Optical Design Dr. John T. Mariska Data Coordination Scientist Naval Research Laboratory
Udo Schühle 5. Solar Orbiter EUS Consortium Meeting RAL, 3. March 2006 EUS NI spectrograph design constraints EUS NI spectrograph design constraints Udo.
Udo Schühle 5. Solar Orbiter EUS Consortium Meeting RAL, 3. March 2006 EUS NI spectrograph design constraints EUS NI spectrograph design constraints Udo.
Science With the Extreme-ultraviolet Spectrometer (EIS) on Solar-B by G. A. Doschek (with contributions from Harry Warren) presented at the STEREO/Solar-B.
1 Estimate on SOT light level in flight with throughput measurements in SOT sun tests T. Shimizu 1, T. Tarbell 2, Y. Suematsu 3, M. Kubo 1, K. Ichimoto.
Géraldine Guerri Post-doc CSL
Physics 681: Solar Physics and Instrumentation – Lecture 7 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
Show 1 -- photosphere & sunspots SUN COURSE - SLIDE SHOW 3 Show 2 -- corona & solar cycle Today: SOHO.
The Solar-B EUV Imaging Spectrometer: an Overview of EIS J. L. Culhane Mullard Space Science Laboratory University College London.
J.P. Halain – Centre Spatial de Liège
Sunspot Studies in Oslo Nils Brynildsen, Per Maltby, Terje Fredvik and Olav Kjeldseth-Moe Institute of Theoretical Astrophysics University of Oslo.
Solar-B Science Objectives - Overview of the Mission - Kazunari Shibata (Kyoto Univ.)
Source lens Entrance slit Exit slit width,  (mm) grating Concave mirrors Focal Plane Focal Length, F (mm)
SDW2005, juin, Taormina The Corot Space instrument.
Rachel Klima (on behalf of the MASCS team) JHU/APL MASCS/VIRS Data Users’ Workshop LPSC 2014, The Woodlands, TX March 17,2014 MASCS Instrument & VIRS Calibration.
ASTRI SST-2M The Prototype monolithic 1.8 m
990901EIS_RR_Instru.1 The Instrument: US Subsystems and Requirements Dr. Clarence M. Korendyke US Project Scientist Naval Research Laboratory
990901EIS_RR_Science.1 Science Investigation Goals and Instrument Requirements Dr. George A. Doschek EIS US Principal Investigator Naval Research Laboratory.
990901EIS_RR_Mgmt_OV.1 Management Overview Dr. George A. Doschek EIS US Principal Investigator Naval Research Laboratory Phone: , FAX:
Optical characteristics of the EUV spectrometer for the normal-incidence region L. Poletto, G. Tondello Istituto Nazionale per la Fisica della Materia.
Grazing-incidence design and others L. Poletto Istituto Nazionale per la Fisica della Materia (INFM) Department of Electronics and Informatics - Padova.
Freiburg, May 2011 EST Design Study. End of Phase-III Meeting European Solar Telescope Design Study End of Phase III Meeting WP Instrument.
THE LHIRES-III SPECTROGRAPH © C2PU, Observatoire de la Cote d’Azur, Université de Nice Sophia-Antipolis Jean-Pierre Rivet CNRS, OCA, Dept. Lagrange
Solar-B Mission Preparation Len Culhane – UK EIS Principal Investigator Louise Harra – UK Project Scientist David Williams – UK EIS Chief Observer Mullard.
SIAMOIS, kickoff meeting, Paris, may, SIAMOIS: optical test bench BOSS (Banc Optique SiamoiS) Pernelle Bernardi Observatoire de Paris-Meudon,
5 Components Common to All Optical Spectrometers Source Transparent Sample Holder Wavelength Selector Radiation Detector Signal Processor and Readout.
EUV Spectroscopy. High-resolution solar EUV spectroscopy.
The Mid-Infrared Instrument (MIRI) Medium Resolution Spectrometer for JWST Martyn Wells MIRI EC & UKATC.
7/12/20011 The STEREO-SECCHI Extreme Ultraviolet Imager J-P. Wülser, J.R. Lemen, T.D. Tarbell, C.J. Wolfson (LMSAL) R.A. Howard, J.D. Moses (NRL) J-P.
The Solar-B EUV Imaging Spectrometer: an Overview of EIS J. L. Culhane Mullard Space Science Laboratory University College London.
High Resolution Echelle Spectrograph for Chinese Weihai 1m Telescope. Leiwang, Yongtian Zhu, Zhongwen Hu Nanjing institute of Astronomical Optics Technology.
Integral Field Spectrograph Eric PRIETO CNRS,INSU,France,Project Manager 11 November 2003.
Space Science Activities at NRL Presentation to the National Space Weather Assessment Committee Herbert Gursky Superintendent, Space Science Division Naval.
20 OCT 2003SOLAR ORBITER MEETING1 Optical Design Activities at RAL Kevin Middleton Optical Systems Group Space Science & Technology Dep’t. Rutherford Appleton.
Apr 17-22, NAOJ External alignment with X-Ray Telescope (XRT) and EUV Imaging Spectrometer (EIS) Y. Katsukawa (NAOJ) and SOT team.
Oct 17, 2001SALT PFIS Preliminary Design Review1 Southern African Large Telescope Prime Focus Imaging Spectrograph Mechanical Mechanism Design Michael.
Optical characteristics of the EUV spectrometer for the grazing-incidence region L. Poletto, G. Tondello Istituto Nazionale per la Fisica della Materia.
Solar orbiter_______________________________________________.
SPACE TELESCOPE SCIENCE INSTITUTE Operated for NASA by AURA SMOV4 Requirements Review Cosmic Origins Spectrograph Scott D. Friedman STScI 30 July 2003.
IFS prototype – PM3 LAM, 13/06/2003 Prototype testing at CRAL Tests at room temperature in the visible.
Oct 17, 2001SALT PFIS Preliminary Design Review Control System 1 Southern African Large Telescope Prime Focus Imaging Spectrograph Preliminary Control.
Sunspot Telescope Sunspots and surface granulation are the two main features. Telescope: Celestron NexStar 5 mounted on a Losmandy mount. Field of View.
06 Oct 05Space Science & Technology Dept1 Solar Orbiter Consortium Meeting 03 Mar 06 Optical Design Of Solar Orbiter Normal Incidence Spectrometer KF Middleton.
Compressor Helium filled optional equivalent plane imaging laser beam dump hole in mirror for e-beam SSA and more.
Spectrometer for Sky-Scanning, Sun-Tracking Atmospheric Research (4STAR) Earth Science Division - NASA Ames Research Center 2006 A concept for a sun-sky.
NIRSpec - the JWST Multi-Object Spectrograph P. Ferruit (ESA), S. Arribas (CSIS), S. Birkmann (ESA), T. Böker (ESA), A. Bunker (Oxford), S. Charlot (IAP),
Date of download: 6/1/2016 Copyright © 2016 SPIE. All rights reserved. Spatial (angular) resolution versus field angle for design with toroidal grating.
Date of download: 6/8/2016 Copyright © 2016 SPIE. All rights reserved. The portions of the datacube collected during a single detector integration period.
3 rd March 2006EUS Consortium meeting EUS Instrument Overview Eric Sawyer RAL.
Solar & Heliospheric Observatory Rayana Thompson & Windell Barfield.
Spectroscopic Observations with SolarB-EIS Helen E. Mason DAMTP, Centre for Mathematical Sciences Giulio Del Zanna, MSSL.
Ben Sheff Development of Optical Metrology ENgine (OMEN)
990901EIS_RR_Tech.1 Overview and Status of EIS Technical Program Dr. Clarence M. Korendyke EIS US Project Scientist Naval Research Laboratory
Integral Field Spectrograph Eric Prieto LAM. How to do 3D spectroscopy.
Single Object Slitless Spectroscopy Simulations
Solar-B Science Working Group
Development of the User Interface for AIR-SPEC
SECCHI Deputy Program Manager
30-Nov-2006 Jean-Marc Defise - CSL
Analyzing and Correcting Stray Light Using LensMechanix
ISAS Solar Physics Yohkoh (1991- ) Hionotori ( )
An IFU slicer spectrometer for SNAP
2018 STCE Annual Meeting Surface UV radiation.
EUS NI spectrograph design constraints
EIS STATUS J.L. Culhane 3rd February, 2003.
BASIC HYPER SPECTRAL IMAGING
Instrument Overview Larry Springer HMI Program Manager
Presentation transcript:

990901EIS_RR_HV.1 Heritage and Validation Approach Dr. Clarence M. Korendyke EIS US Project Scientist Naval Research Laboratory

990901EIS_RR_HV.2 EIS Component and Design Heritage Scan Mirror Design: SUMER/LASCO Motor Actuators: Distributed List Includes HST and UVCS Shutter Design/Actuators: MDI, TRACE, SXI PZT: Flight Heritage on LASCO Fabry-Perot and M1 Tilt Mechanism Bearings and Slides: HRTS and SUMER Optical Design Heritage: EIT, TRACE, CDS, SUMER and SERTS

990901EIS_RR_HV.3 Environmental Test

990901EIS_RR_HV.4 Optical Component Test

990901EIS_RR_HV.5 NRL Beamline X24-C at NSLS Synchrotron

990901EIS_RR_HV.6 End to End Test Focus and Image Quality Testing of the Telescope Will Be Conducted in the Visible Using a Collimator and Slit Plane Imaging System –This Test Will Follow the Procedures Successfully Implemented in the AS&E and HRTS Rocket Programs Spectrometer Focus and Image Quality and Spectral Line Profile Testing Will Occur at EUV Wavelengths Using a Modified Supplier’s Collimator End-to-End Image Quality Test Will Be Conducted With the NRL’s Collimator End-to-end Calibration Scans of the Entrance Aperture With a Standard Source at RAL Will Be Conducted –This Test Will Follow the Standard Procedures Developed for CDS and SERTS –Results of This Test Will Be Used to Correct the Instrument Response Profile in Absolute Magnitude Visible Rejection Test With a Heliostat or Appropriate Simulated Solar Source Will Be Conducted

990901EIS_RR_HV.7 NRL-Generated Interface Memoranda