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.

Slides:



Advertisements
Similar presentations
Grazing-incidence vs. normal-incidence design L. Poletto CNR - National Institute for the Physics of Matter Department of Information Engineering - Padova.
Advertisements

THROUGHPUT OF A NORMAL INCIDENCE SPECTROMETER DESIGN IN DIFFERENT WAVELENGTH RANGES Luca Teriaca Max Planck Institut für Sonnensystemforschung.
HIRES Technical concept and design E. Oliva, HIRES meeting, Brera (Milan, Italy)1.
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.
The waves spread out from the opening!
PSI: Polarimetric Spectroscopic Imager - A Simple, High Efficiency, High Resolution Spectro-­Polarimeter Samuel C. Barden Frank Hill.
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.
Optical Astronomy Imaging Chain: Telescopes & CCDs.
PACS IIDR 01/02 Mar 2001 Baffle and Straylight1 D. Kampf KAYSER-THREDE.
Solar Orbiter EUV Spectrometer
AURA New Initiatives Office S.C. Barden, M. Liang, K.H. Hinkle, C.F.W. Harmer, R.R. Joyce (NOAO/NIO) September 17, 2001 Instrumentation Concepts for the.
Direction-detection spectrometer concepts the CCAT Matt Bradford + others 24 October 2006, in progress.
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.
1 A Grating Spectrograph for the LCLS Philip Heimann Advanced Light Source Observe the spontaneous radiation spectrum of the individual undulators Observe.
R. M. Bionta SLAC November 14, 2005 UCRL-PRES-XXXXXX LCLS Beam-Based Undulator K Measurements Workshop Use of FEL Off-Axis Zone Plate.
Source lens Entrance slit Exit slit width,  (mm) grating Concave mirrors Focal Plane Focal Length, F (mm)
Monochromator Improvements and Focusing Elke Jackson Research performed by Elke Jackson, Shannon Lunt, and Yenny Martinez With the support of Drs. Steven.
Astronomical Spectroscopy
990901EIS_RR_Science.1 Science Investigation Goals and Instrument Requirements Dr. George A. Doschek EIS US Principal Investigator Naval Research Laboratory.
Optical characteristics of the EUV spectrometer for the normal-incidence region L. Poletto, G. Tondello Istituto Nazionale per la Fisica della Materia.
Optical characteristics of the EUV spectrometer (EUS) for SOLO L. Poletto, G. Tondello Istituto Nazionale per la Fisica della Materia (INFM) Department.
Optical Design for an Infrared Multi-Object Spectrometer R. Winsor, J.W. MacKenty, M. Stiavelli Space Telescope Science Institute M. Greenhouse, E. Mentzell,
Science Specification of SOLAR-C payload SOLAR-C Working Group 2012 July 23.
EUV Spectroscopy. High-resolution solar EUV spectroscopy.
MCAO Adaptive Optics Module Subsystem Optical Designs R.A.Buchroeder.
Engineering: NAHUAL Ireland Acquisition Camera, Focal Plane Mechanisms and Layout Tully Peacocke, National University of Ireland Maynooth Carlos del Burgo,
PACS IIDR 01/02 Mar 2001 FPFPU Alignment1 D. Kampf KAYSER-THREDE.
Telescopes & recent observational techniques ASTR 3010 Lecture 4 Chapters 3 & 6.
14 October Observational Astronomy SPECTROSCOPY and spectrometers Kitchin, pp
Near Infrared Spectro-polarimeter (NIRSP) Conceptual Design Don Mickey Jeff Kuhn Haosheng Lin.
TESIS on CORONAS-PHOTON S. V. Kuzin (XRAS) and TESIS Team.
18 October Observational Astronomy SPECTROSCOPY and spectrometers Kitchin, pp
An IFU for IFOSC on IUCAA 2m Telescope
CLIC meeting Jan Kovermann. Task: Analysis of the light which is emitted by a breakdown Study the breakdown time dependence of the BD light emission.
Warm-up Find the circumference and area of the following circles: R = 7 ft D = 20 in.
The waves spread out from the opening!
20 OCT 2003SOLAR ORBITER MEETING1 Optical Design Activities at RAL Kevin Middleton Optical Systems Group Space Science & Technology Dep’t. Rutherford Appleton.
Optical characteristics of the EUV spectrometer for the grazing-incidence region L. Poletto, G. Tondello Istituto Nazionale per la Fisica della Materia.
Solar orbiter_______________________________________________.
Science with Giant Telescopes - Jun 15-18, Instrument Concepts InstrumentFunction range (microns) ResolutionFOV GMACSOptical Multi-Object Spectrometer.
Model instruments baseline specification and key open issues EUV/FUV High-Throughput Spectroscopic Telescope Toshifumi Shimizu (ISAS/JAXA) SCSDM-4.
020625_ExtReview_Nexus.1 NEXUS / SDO / ILWS SDO Science goals: How does solar variability directly affect life on Earth? SDO areas of interest: –Solar.
Visible Spectro-polarimeter (ViSP) Conceptual Design David Elmore HAO/NCAR
STC "VOSKHOD", PROJECT "SPECTR-UV", JUNE 2006 Next slide Next slide Previous slide Possible layouts of Field Cameras.
N A S A G O D D A R D S P A C E F L I G H T C E N T E R I n t e g r a t e d D e s i g n C a p a b i l i t y / I n s t r u m e n t S y n t h e s i s & A.
Normal-Incidence Design Option for SolO/EUS Roger J. Thomas NASA/GSFC 2004 November 04.
Spectrometer Throughput Dr Peter Young Consortium meeting, 3 March 2006.
06 Oct 05Space Science & Technology Dept1 Solar Orbiter Consortium Meeting 03 Mar 06 Optical Design Of Solar Orbiter Normal Incidence Spectrometer KF Middleton.
PACS IIDR 01/02 Mar 2001 Optical System Design1 N. Geis MPE.
990901EIS_RR_HV.1 Heritage and Validation Approach Dr. Clarence M. Korendyke EIS US Project Scientist Naval Research Laboratory
Date of download: 6/1/2016 Copyright © 2016 SPIE. All rights reserved. Spatial (angular) resolution versus field angle for design with toroidal grating.
3 rd March 2006EUS Consortium meeting EUS Instrument Overview Eric Sawyer RAL.
Spectroscopic Observations with SolarB-EIS Helen E. Mason DAMTP, Centre for Mathematical Sciences Giulio Del Zanna, MSSL.
Integral Field Spectrograph Eric Prieto LAM. How to do 3D spectroscopy.
CASE spectrograph Spectrograph Optical Specifications
Astronomical Spectroscopic Techniques
LAI-FKSI Optical Sensitivity at 2µ wavelength
MEASUREMENT OF THE WAVELENGTH OF MONOCHROMATIC LIGHT
An IFU slicer spectrometer for SNAP
First Assessments of EUVI Performance on STEREO SECCHI
EUS NI spectrograph design constraints
EIS STATUS J.L. Culhane 3rd February, 2003.
Quiz_03 2-slits interference, Phasor, thin film interference
Diffraction Grating calculation of light wavelength
Optics Alan Title, HMI-LMSAL Lead,
Presentation transcript:

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 micron pixels Two Wavelength Bands of 40 Å width –Short Wavelength Centered at 190Å –Long Wavelength Centered at 270Å Two Detectors cover 40Å each 4800 l/mm grating- Single Ruling Density –Half ML Coated for 190Å –Half ML Coated for 270Å Detector Must Clear Input Path (etc.)

EIS-7Tr Design Heritage Trendy: Paraboloid Telescope –Only two reflections SERTS: Toroidal Grating J-PEX: Laminar Rulings EIS & Trace: Sectored Multilayer Coatings Sumer: Primary Mirror Scan Concept

EIS-7TR Spectrometer Layout Grating Slit 190A 270A

EIS-7TR Spectrometer Layout 270 A Band

EIS-7Tr Spot Diagrams & Histograms