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HIRDES PhaseB1 Kayser Threde FinalPresentation - PowerPoint PPT Presentation

HIRDES PhaseB1 Kayser Threde FinalPresentation www.kayser#threde.com @DLR,Bonn April05,2006 R.Graue;D.Kampf;Ch.Neumann Contents Requirements PhaseB1Study Logic SystemArchitecture Optical


  1. HIRDES Phase�B1 Kayser Threde Final�Presentation www.kayser#threde.com @DLR,�Bonn April�05,�2006 R.�Graue;�D.�Kampf;�Ch.�Neumann

  2. Contents � Requirements � Phase�B1�Study Logic � System�Architecture � Optical Performance � Mechanical and�Structural Design � Thermal�and�Distortion Analyses � Mechanisms Design � In�Orbit�Calibration � Electronics�and�Detectors � Budgets � Design,�Development and�Verification Plan � Documentation 2 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  3. HIRDES�Requirements 3 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  4. HIRDES�Instrument�– Driving�Requirements Parameter Baseline�Requirements Wavelength�coverage � UV�Spectrograph 1748310�nm � VUV�Spectrograph 1028176�nm Spectral�Resolution >�48000 Minimum�sensitivity � SNR=�10�in�10�h 16�mag (VUVES);�18�(UVES) � SNR=�100�in�10�h 11�mag (VUVES);�13�(UVES) Limit�loads�in�all�axes�w/o�SF 15�g�(tbc) Stiffness�(first�fundamental�eigenfrequency) >�40�Hz Envelope� Protective�Case Mass 155�kg Power 150�W Data�Rate�(downlink) 1.6�Mbit/sec 4 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  5. Applicable Documents AD1 User�Requirements Document;�3.2006 AD2 Project�WSOUV�;�Phase�A�Preliminary Design(T170�M)�;�7.2005 5 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  6. Phase�B1�Study�Logic 6 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  7. Main�Objectives�of�the�HIRDES�Phase�B1�Study � System�Architecture�and�Design�Conceptual�Design � Preliminary Engineering� � Optical Performance�of�Spectrometers and�IFGS � Structural Performance� � Mechanical Configuration and�Conceptual Design � Thermal�Behaviour and�Optical Stability � Electronics�and�Software�Architecture � MCP�/�IFGS�Detector Performance�Analyses�and�Design� � External�IF�Engineering�(Telescope,�External�Electronics�Panels) � Evaluation�of�Programmatic� � Design,�Development�and��Verification�Plan � PA�Approach� � ROM�Cost�Estimations 7 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  8. Architectural�Trades�and�Engineering�# Overview � Optical Analyses and�Layout�(Spot�Diagrams,�Ray�Tracing) � Thermal�Analyses and�Control (Passive,�Active) � Structural Analyses (Eigenmodes,�Strength) � Performance�Analyses (Distortion Analyses,�Tolerancing) � Mechanical Design� � Mechanisms Concept � MCP�and�IFGS�Detector Design � Instrument�Electronics�Design � IF�Engineering�to�S/C�(Telescope,�Electroics) � Budgets�(Mass,�Power,�Data) � In�Flight Calibration Concept >tbc 8 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  9. Study Logic Phase�B1 KO Architectural Design� ICD�preparation PM1 Preliminary Design�and�Engineering DDV�Plan�and�ROM�Cost Estimation Preliminary Documentation FP (DLR) Final�Documentation 9 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  10. Phase�B1�Team�Configuration IAAT Scientific and�Technical Management MCP�Detector Engineering�Support KT ISAS Industrial�Study Team Scientific Consultancy Optomechanics,�Electronics Spectrometer Layout� Expertise 10 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  11. 11 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  12. System Architecture 12 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  13. T�170�M�Telescope 13 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  14. Baseline�Configuration�of�HIRDES�(VUVES�and�UVES)� � Phase�A�� � UV�and�VUV�Spectrometers�Optomechanics (Optical�Elements,�Housing) � UV�and�VUV�MCP�Detectors�(2�x�2)�including�Front�End�Electronics� � ICU�(Instrument�Control�and�Data�Processing)� � HVPS�and�LVPS�(High�and�Low�Voltage�Power�Supply) � Thermal�H/W� � Mechanisms�including�Motor�Control�Electronics � Vacuum�Shutter�for�MCP�Detectors�(UV,�VUV) � Grey�Filter�Mechanism�(UV,�VUV) � Servo�Mirror�Mechanism�(UV,�VUV) � Echelle and�Collimator�Focus�Mechanisms�(UV,�VUV) � Phase�B1�(Additional�Equipment) � UV�and�VUV�Internal�Fine�Guidance�Sensor�(IFGS)�including�Front�End�Electronics� and�Optics 14 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  15. Optical Performance 15 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  16. HIRDES�Optical�Layout�incl.�WSO/UV�Telescope�T170M VUV�Spectrometer UV�Spectrometer T170�M�Telescope � Focal�Length:� 27�m � Primary�Mirror:� dia.�1.7�m 16 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  17. UV�Spectrograph UV�spectrograph with echelle grating (40�lines/mm�/�70deg.blaze)� and�prism (fused silica,�12�deg.) 17 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  18. UV�Spectrograph�# Focal�Plane Wavelength : 174#312�nm Grating order 253#149 18 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  19. UV�Spectrograph�# Focal�Plane�High�Resolution�(69000) Spots�at�position 5�for demonstration only 19 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  20. UV�Spectrograph�# In�Field�Fine�Guidance�with�Lens In�field reflected at�prism front�surface towards focus mirror via�lens onto fine�guidance detector 20 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  21. UV�Spectrograph�# In�Field�Fine�Guidance�Performance�with�Lens • Spots�at�550�nm�with�10�Bm�pixel�and�0.3�arcsec distance�(instant�illumination) • Spots�ranging�at�600�and��630�nm�with�10�Bm�pixel�and�0.3�arcsec distance�(instant�illumination) 21 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  22. VUV�Spectrograph Spectral separation via�echelle grating (65�lines/mm/71�deg.�blaze)� and�cross�disperser (on�focus mirror,�625�lines/mm) 22 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  23. VUV�Spectrograph�# Focal�Plane Wavelength: 102#176�nm Grating order: 282#165 23 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  24. VUV�Spectrograph�# In�Field�Fine�Guidance In�field decoupled from 0th�order�reflection of�grating via�2�mirrors onto fine�guidance detector 24 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  25. VUV�# In�Field Fine�Guidance # Performance � Spots,�10�Bm�pixel � 2�spots�with�10Bm�pixel�and�0.6�arcsec distance�(instant�illumination�for�demonstration�only)� � Diffraction�limitation�due�to�600nm�wavelength�and��160�m�focal�length�(diffraction�limited) 25 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  26. Mechanical and�Structural Design 26 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  27. HIRDES�Spectrometer�Primary�Structure�# Baseline � Modular�Approach�of�Spectrometer�Housing�(Stand�Alone�Spectrometer�Units) � Monolithic�CeSiC structure�(conservative�material,�quasi�isotropic�behaviour) � Light#weight�approach � Minimized�Procurement�costs� � Fabrication�technology�available�in�Germany� � Reduced�Manufacturing�tolerances � Standardized�adjustment�devices�for�each�optical�component � Isostatic suspension�for�the�HIRDES�spectrometers�to�the�Telescope�I/F � Isostatic suspension�and�thermal�decoupling�between�detectors�and�Spectrometer� Housing 27 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  28. Spectrometer�Arrangement B B 50 1100 LSS 0 1 2 A UV�Spectrometer 120 ( � 3x ) 3 7 . 3 U V h Spect r om et er 540 Y Z 520 VU V Spect r om et er 462 ( � 3x ) O pt i cal � bench� I / F see� page� 2 VUV�Spectrometer A 28 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  29. Critical�Components��Design Mirrors�and�Gratings� • Quartz�Glas with�Invar�flexural�mounts • WFE:� λ λ /20�at� λ λ =�633�nm λ λ λ λ • Surface�Roughness:� <�1�nm • Coatings:� • UV�:�Al�+�SiO 2 • VUV:�Al�+�MgF 2 • VIS:�Al�+�SiO 2 (Option:�Au) Isostatic Mirror�Suspension (ORFEUS�Heritage) 29 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

  30. Critical�Components��Design Isostatic Suspension�made�from�CFRP Invar�Suspension�with�SS�flexural�Blades (PACS�heritage) (ORFEUS�Heritage) 30 HIRDES�Final�Presentation�;�05.04.2006,�DLR HIRDES

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