Confidence through traceability

Size: px

Start display at page:

Download "Confidence through traceability"

Martina Smith
5 years ago
Views:

1 Confidence through traceability 1 st November 2016 The Institute of Engineering and Technology

2 Dr Peter Thompson, NPL CEO Alan Turing s Pilot ACE

3 Dr Peter Thompson, NPL CEO NPL Miniature Atomic Clock World s first atomic clock

4 Prof Paul Shore, NPL Engineering Measurements Division NPL High Accuracy Indoor GPS Confidence through traceability

LINK Nanotechnology Programme 1988-1994 Project

$refractometer high accuracy laser interferometry$

6 LINK Nanotechnology Programme Project 01- NION Ultra Precision Machine NPL refractometer high accuracy laser interferometry Courtesy of Cranfield University Confidence through traceability

7 James Webb Space Telescope MIRI INSTRUMENT Image slicers Produced for UK ATC Courtesy of Cranfield University

8 James Webb Space Telescope Colin Cunningham UK Astronomy Technology Centre Royal Observatory Edinburgh 8

9 Mirror diameter 6.5 metres L2 orbit (1 million miles from Earth in the anti-sun direction) Optics passively cooled to 40K - allows sensitive performance at infrared wavelengths.

10 JWST Science Overview M81 First Light and Re-Ionization HH-30 Assembly of Galaxies GL146 Birth of stars and proto-planetary systems Planetary systems and the origin of life

11 JWST will have 4 Science Instruments Low resolution slitless spectroscopy

12 The MIRI Partnership

filter Output slitets Roof mirror Light trap WHEEL A Adjustable fold mirror

13 Engineering Complexity MIRI spectrometer and image slicers Image slicer mirror APO output fold M3 M1 INPUT MIRROR CHANNEL 1 APO Pupil images M4 M2 INPUT Blocking filter Output slitets Roof mirror Light trap WHEEL A Adjustable fold mirror Re-imaging mirror array D1 D2 D3 CHANNEL 2 APO Fold mirror WHEEL B Light trap CHANNEL 3 exit port

14 Integral Field Spectroscopy: 3D data cube Image: Stephen Todd and Douglas Pierce-Price

15 Image courtesy of Niranjan Thatte, Oxford

16 Image Slicer Image slicer mirror APO output fold M3 M1 Pupil images M4 M2 INPUT Output slitets Roof mirror Re-imaging mirror array

17 JWST MIRI image slicer and re-imaging mirrors Manufactured by Cranfield University using the CUPE NION Nanocentre

18 CUPE Nanocentre Diamond Turning System (1988) Funded by the 1 st DTI Link Nanotechnology project

19 5 nm roughness rms MIRI Slicer verification model channel 1 10 nm rms form accuracy Recent test results show very low errors due to scattering at the edges

20 MIRI during temperature alignment testing at RAL Copyright: Stephen Kill, STFC

21 MIRI on its way to Goddard Space Flight Center on May 29 th 2012

22 ISIM MIRI Copyright: NASA/Goddard Space Flight Center/Chris Gunn

23 JWST coming together for launch in 2018 Acknowledgements: Gillian Wright: MIRI European PI, NASA, ESA, Cranfield Univ

24 Prof Ian Boyd, Chief Scientific Advisor NPL DIAL emission monitoring mobile lab NPL Solar Radiometer NPL Cryogenic Radiometer Confidence through traceability

25 Prof Neil Stansfield, Strategic Lead, Quantum Technology Programme Mark Wagner - ESTEC 11/01/2016 Slide 25 ESA UNCLASSIFIED - For Official Use Confidence through traceability

26 THE EUROPEAN SPACE AGENCY November 2016 ESA UNCLASSIFIED - For Official Use

27 Issue/Revision: 1.0 Reference: - Status: N/A ESA UNCLASSIFIED - For Official Use

28 Mark Wagner - ESTEC 11/01/2016 Slide 28 ESA UNCLASSIFIED - For Official Use

29 Mark Wagner - ESTEC 11/01/2016 Slide 29 ESA UNCLASSIFIED - For Official Use

30 Mark Wagner - ESTEC 11/01/2016 Slide 30 ESA UNCLASSIFIED - For Official Use

31 Mark Wagner - ESTEC 11/01/2016 Slide 31 ESA UNCLASSIFIED - For Official Use

32 Mark Wagner - ESTEC 11/01/2016 Slide 32 ESA UNCLASSIFIED - For Official Use

33 DMC-3 image: Credit SSTL Mark Wagner - ESTEC 11/01/2016 Slide 33 ESA UNCLASSIFIED - For Official Use

34 Mark Wagner - ESTEC 11/01/2016 Slide 34 ESA UNCLASSIFIED - For Official Use

NPL Menu Micro-Newton thrust balance Voice coil actuators Calibration soup Hot current source Micro-vibration hotpot Uncertainty budget mixed Seismometer pie

35 NPL Menu Micro-Newton thrust balance Voice coil actuators Calibration soup Hot current source Micro-vibration hotpot Uncertainty budget mixed Seismometer pie Interferometer mash Traceability ragout Repeatability and cross-talk Negative stiffness Mark Wagner - ESTEC 11/01/2016 Slide 35 ESA UNCLASSIFIED - For Official Use

36 Mark Wagner - ESTEC 11/01/2016 Slide 36 ESA UNCLASSIFIED - For Official Use

37 Mark Wagner - ESTEC 11/01/2016 Slide 37 ESA UNCLASSIFIED - For Official Use

38 Mark Wagner - ESTEC 11/01/2016 Slide 38 ESA UNCLASSIFIED - For Official Use

39 Mark Wagner - ESTEC 11/01/2016 Slide 39 ESA UNCLASSIFIED - For Official Use

40 Mark Wagner - ESTEC 11/01/2016 Slide 40 ESA UNCLASSIFIED - For Official Use

41 Mark Wagner - ESTEC 11/01/2016 Slide 41 ESA UNCLASSIFIED - For Official Use

43 Mark Wagner - ESTEC 11/01/2016 Slide 43 ESA UNCLASSIFIED - For Official Use

44 Dan Veal, NPL NPL Instruments Group Leader Unique bespoke instrument supplier for industry, science and innovation organisations >600 leading measurement scientists Traceability authority ISO9000 design, build and supply Opto-mechatronic expertise CAD/CAM precision engineering capacity with leading partners Confidence through traceability

45 How to work with us? Confidence through traceability

46 Supper and discussions Confidence through traceability

MATRIX-MG Series. Innovation with Integrity. Automated High-Performance Gas Analyzers FT-IR

MATRIX-MG Series. Innovation with Integrity. Automated High-Performance Gas Analyzers FT-IR MATRIX-MG Series Automated High-Performance Gas Analyzers Innovation with Integrity FT-IR The MATRIX-MG Series comprises three high-performance FT-IR gas analyzers in a compact and rugged housing. They