Survey
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Company profile & Space Science Detector Capabilities - Ian Cox www.photek.co.uk page 1 Company Profile • Specialist manufacturers of vacuum based detectors and camera systems for photon detection. Photek manufacture Image Intensifiers, PMT’s, Streak Tubes, open faced detectors and a range of associated electronics and camera systems • Located in St Leonards-on-Sea – South East England • Established September 1991 www.photek.co.uk page 2 Company Profile • 36 Employees – 10 sales/administrative – 7 R&D – 19 production/test • 5 employees educated to PHD level • Further 8 employees educated to degree level www.photek.co.uk page 3 Detector Products • MCP image intensifier • Ultra fast MCP photomultipliers • Streak tubes • Magnetic focus image intensifiers • De-magnifying gen 1 image intensifiers • Vacuum compatible detectors www.photek.co.uk page 4 Camera Products • Photon counting • Nanosecond ICCD • Intensified CCD • Fluorescence • X-ray • Particle imaging www.photek.co.uk page 5 Electronic Products • HT power supplies • Nanosecond gating control • Laser pulse generator • Preamplifier • Image intensifier cooling www.photek.co.uk page 6 Applications • Early warning Missile systems • Wafer silicon inspection • Astronomy including orbital space science experiments • Ultra-high speed cameras • Nuclear & high energy physics research • Life-science research • Industrial processing • Security www.photek.co.uk page 7 Facilities • 1,500m2 factory space • Class 100 assembly area • Class 10,000 clean room • Electro-mechanical vibration table • Ultra-high vacuum processing equipment • High speed (50 ps) laser pulsing equipment • Wet and dry hydrogen stoving capability • Inventor 3-D CAD software www.photek.co.uk page 8 Facilities – Continued • Protel Electronic Design Software • Agilent 18 GHz sampling scope • LeCroy 5 GHz digital scope • Spectrometer • Photometer • Optical table and dark room facilities • Environmental test chamber • Phosphor screen production and inspection facilities • Optical coating plant www.photek.co.uk page 9 Quality • Photek operates a company wide quality system based on ISO9000 and TQM principles • Currently working towards ISO9000 accreditation with successful implementation expected in 2008 • We operate a strict stock control and inspection policy with all items batch controlled and tracked • All detectors and systems are fully characterised in out photometry laboratory • Each device has a serial number that is used throughout the entire manufacturing process www.photek.co.uk page 10 Test and Support • Excellent support and test facilities • Rigorous testing of all products is completed before release • Support question always answered by a technical member of staff. Typically educated to PHD level • 12 month warranty on all products • Technical support for lifetime of product www.photek.co.uk page 11 Space Science Projects • ACE Advanced Composition Explorer • XMM UV Optical Monitor • MSX UVISI Detector • GUVI Global Ultraviolet Imager • SSUSI Special Sensor Ultra-violet Spectrographic Imager • UVIT Ultra-Violet Imaging Telescope www.photek.co.uk page 12 Advance Composition Explorer • CRIS Detector (Cosmic Ray Isotope Spectrometer) – 40 mm Image Intensifier with 2 MCP – UV Fibre Optic Input Window – Blue Enhance Cathode to Match Scintillating Fibre Optics – • 100,000 Gain Uses scintillating fibre optic structure. The detector is to measure direction and energy of cosmic rays www.photek.co.uk page 13 UV Optical Monitor • Photon Imaging 170 nm to 550 nm region • Aligned with X-Ray Telescope • Provides Simultaneous Visible, UV and X-ray Images www.photek.co.uk page 14 The XMM Detector • 25 mm Photon Counting • High Sensitivity in the 170 nm to 550 nm Region • Built in Fibre Optic Taper • Concave Input Window www.photek.co.uk page 15 Mid Course Space Experiment • Johns Hopkins University • Launched 24 April 96 • Part of the spectrograph on the UVISI Instrument • Diffuse and Discrete Aurora • Low Earth Atmosphere Phenomena www.photek.co.uk page 16 MSX-UVISI Detector • 40 mm Photon Counting Image Intensifier • MgF2 Input Window • CsI Photocathode • 100 nm – 250 nm Response www.photek.co.uk page 17 Global Ultra Violet Imager • Johns Hopkins University Applied Physics Laboratory • Launched on the TIMED Spacecraft during 2001 • TIMED is used to study the energetics and dynamics of the Mesosphere and lower Thermosphere between an altitude of approximately 60 to 180 kilometers. • GUVI is a far-ultraviolet (115 to 180 nm), scanning imaging spectrograph that provides horizon-tohorizon images in five selectable wavelength intervals www.photek.co.uk page 18 GUVI Detector • 25 mm UV Photon Counting • MgF2 Input Window • CsI Photocathode • Wedge and Strip Anode • 106 cps • 3x106 Gain www.photek.co.uk page 19 Ultra-Violet Imaging Telescope • Indian Space Research Organisation (ISRO) • Due to launch on the ASTROSAT spacecraft during 2008 – now delayed until 2012. • ASTROSAT aims are to investigate the origin and mechanism of radiation emissions in active galactic nuclei. • UVIT aims to provide flux calibrated images of the sky in the far-UV, near-UV and visible spectral regions www.photek.co.uk page 20 Summary • World leading space science vacuum detector manufacturer • Photek have the experience and knowledge to produce detectors to the most stringent space science requirements • Quality systems in place to ensure repeatability of detector manufacture • Test and support facilities give first class support for the lifetime of our detectors www.photek.co.uk page 21 UVIT Detectors • Three 40 mm photon counting detectors • Far UV (120-180 nm) • Near UV (180-300 nm) • Visible (180-550 nm) • Integrated fibre optic taper with bonded FillFactory Star 250 CMOS sensor www.photek.co.uk page 22 UVIT Detectors Photek have supplied 7 detectors for the UVIT project • NUV EM • NUV FM and FS • FUV FM and FS • VIS FM and FS www.photek.co.uk page 23 UVIT Detector www.photek.co.uk page 24 Outline Specification FUV Detector 120-180nm • MgF2 Input Window •CsI Solar Blind Photocathode •2x 60:1 40mm MCP’s •P46 Phosphor •Fibre taper output •Star250 Sensor NUV Detector 180-300nm •Fused Silica Input Window •CsTe Solar Blind Photocathode VIS Detector 180-550nm •Fused Silica Input Window •Low Noise S20 Photocathode www.photek.co.uk page 25 Spectral Response Wavelength Specification QE Measured QE 120nm >5.8% 6.8% 7.3% 130nm 140nm >6.2% 5.3% 150nm 160nm >4.2% 4.3% 3.5% 170nm 180nm 6.2% >1.2% 1.2% 190nm 0.5% 200nm 0.2% www.photek.co.uk page 26 Cathode Recess Position Recess (mm) A 2.067mm B 2.056mm C 2.047mm Centre 2.050mm The cathode recess is measured from the front of the DM mounting ring and the front of the input window. A B C www.photek.co.uk View from front of detector page 27 Window Thickness Position Optical Thickness (mm) A 3.6mm B 3.6mm C 3.6mm Centre 3.6mm The window thickness is an optical measurement from the photocathode surface to the outside surface of the window. A B C www.photek.co.uk View from front of detector page 28 Cathode to MCP Gap Position Gap (mm) A 0.11mm B 0.11mm C 0.10mm Centre 0.11mm The cathode gap is measured from the photocathode surface of the input window to the front of the MCP A B C www.photek.co.uk View from front of detector page 29 Electrical – Operating Voltages Optimal Maximum O/V Test Cathode -270V -270V -300V MCP 2350V 2600V 2860V Anode 5000V 5500V 6000V • Cathode and MCP voltage WRT ground (MCP Input). • Anode voltage WRT MCP output. • Optimal voltages are voltages as tested at Photek • The maximum specified voltages should not be exceeded • Each electrode has been over voltage (O/V) tested to the stated value www.photek.co.uk page 30 Resolution Wavelength Cathode Voltage Resolution 185nm -300 20 microns FWHM www.photek.co.uk page 31 FUV FM Gain Calibration -100V Nominal Cathode MCP Anode -270V 2580V 3500V Cathode MCP Anode -270V 2480V 4000V Cathode MCP Anode -270V 2400V 4500V Cathode MCP Anode -270V 2350V 5000V Cathode MCP Anode -270V 2300V 5500V www.photek.co.uk -50V Nominal +50V +100V page 32 Event Size Cathod e MCP Anode -100V -50V Nominal +50V +100V -270 2580 3500 1.9 1.9 2 2.1* 2.2* -270 2480 4000 1.8 1.8 1.9 1.9 2 -270 2400 4500 1.7 1.7 1.8 1.8 1.9 -270 2350 5000 1.6 1.7 1.7 1.8 1.8 -270 2300 5500 1.6 1.6 1.7 1.7 1.8 Note: The approximate FWHM of the event footprints has been measured and the results shown above for a range of operating voltages. www.photek.co.uk page 33 Dark Noise Count rate graph shows variation of count rate on a 1 second timescale. 2 Hour Dark Noise Image @22C No bright defects detectable Average rate 5cps www.photek.co.uk page 34 Image Alignment A B C D View from front of detector www.photek.co.uk Star250 Readout page 35 Uniformity Horizontal / vertical cathode uniformity Average uniformity SD/Mean=4.5% www.photek.co.uk page 36 Environmental Testing 1. 2. 3. 4. 5. 6. 7. 8. Encapsulation of detector 24 Hour / 40C Bake to cure Arathane Qualification level thermal cycle Bond Star250 sensor Vacuum Test Acceptance level thermal cycle Acceptance level vibration tests Final acceptance tests Note: Detector is tested after each stage of environmental testing www.photek.co.uk page 37 Vacuum Test Photek do not have full thermal vacuum test facilities. The following compromise test was agreed: 1. 2. 3. 4. Place detector in a vacuum chamber Leave for 24 hours @20C Increase the room temperature to 30C and leave for 48 hours Reduce room temperature back to 20C and leave for 24 hours www.photek.co.uk page 38 Thermal Cycle Qualification Level Thermal Cycle +35˚C -15˚ C +45˚C -25˚C Peaks Acceptance Level Thermal Cycle +30˚C -10˚C +40˚C -20˚C Peaks Note: Short cycles 2hrs, long cycles 24 hrs www.photek.co.uk page 39 Sine Vibration 100.0 LogMag, g 10.0 1.0 100.0m 5.0 10.0 100.0 Frequency, Hz Frequency (Hz) Acceptance level 5 – 20 8.3mm (0-Peak) 20 – 50 13.3g 50 – 70 10g 70 –100 5.3 g Sweep rate 4 oct. / min. www.photek.co.uk page 40 Random Vibration 1.0 LogMag, g²/Hz 100.0m 10.0m 1.0m 20.0 100.0 1.0K 2.0K Hz Frequency (Hz) Acceptance Level PSD (g2 / Hz) 20 – 100 + 3 dB / oct. 100 – 700 0.09 700 – 2000 - 6 dB / oct. Overall RMS 9.9 g www.photek.co.uk page 41 Thank you for listening www.photek.co.uk page 42