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Visible and UV CCD detectors

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TCP/IP based remote testing, programming, diagnostics, and ... proof-of-principle for the UVCI coronagraph, which is in the ESA Solar Orbiter mission baseline ... – PowerPoint PPT presentation

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Title: Visible and UV CCD detectors


1
Visible and UV CCD detectors
Università degli studi di FirenzeDip. di
Astronomia e Scienza dello Spazio
Luca Gori
2
Summary
XUVLab CCD-CMOS electronics software for
ground- and space-based applications
  • Innovative features of our detectors
  • Software characteristics
  • CCD camera / computer interfaces
  • Current application HERSCHEL sub-orbital mission

3
Innovative features
  • Our philosophy
  • Versatility 1 camera ? n applications
  • Customizable
  • High modularity, upgradeable
  • TCP/IP based remote testing, programming,
    diagnostics, and image acquisition
  • High performance (low noise, high dynamic range,
    slow scan or high frame rate)
  • Great care in the customer support
  • Additional outputs to manage auxiliary devices
  • Compact and low power instrument, portable
    version with air- or fluid-cooled, Peltier
    available

4
Main features
  • Support of CCD formats up to 40964096 pixel
  • Low noise proxy electronics (1.8 nV/vHz rms)
  • Minimum cooling temperature -75C (Peltier)
  • PT100 temperature sensor in the cold finger
  • Air- or fluid-cooled Peltier with closed-cycle
    fluid circulation available
  • Quartz window, windowless or C-type objective
  • High vacuum compatible (10-7 mbar)
  • Tunable pixel rate up to 10 Mpixel/s
  • 9 clocks (-13V to 18V), 10 bias (-3V to 33V)
    available to allow easy interface with any CCD
  • Dynamic range 16 bit _at_ 2 Msample/s
  • Wavelength range NIR, VIS, UV, soft-X ray, X-ray

5
Software interface
6
Software interface
Software interface LabVIEW6i based proprietary
interface
  • Easy and user-friendly interface
  • Quick setting of all configuration parameters
    (CCD format, clock timing, exposure time, pixel
    rate,...)
  • Images display, processing and storage
  • Automatic and continuous acquisition procedures
    with varying pixel rate and exposure time
  • Remote control (TCP/IP protocol)
  • Continuously SW tunable pixel rate
  • Exposure time Normal 1 ms to 17 min (1 ms
    step) Astronomy 1 s to hours (1 s step)
  • Programmable pixel binning
  • OS platform Windows, Unix, Linux, MacOS
  • CCD Timing Software selectable up to 4 parallel
    and serial clocks

7
CCD camera / computer interface
Available configurations
  • PCI data acquisition board SCSI cable
  • SpaceWire protocol

Configurations under study
Fast serial protocols (USB 2.0,
FireWire) Wireless communication
8
HERSCHEL (SCORE) suborbital mission
9
HERSCHEL (SCORE) suborbital mission
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