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SPIRE instrument Flight Model
SPIRE instrument Flight Model - Credits RAL
SPIRE
The instrument is composed of:
An imaging photometer
A FTS spectrometer
SPIRE Warm electronics flight model
SPIRE Warm Electronics flight model on HSO satellite pannel - Credits RAL
SPIRE FPU integration on the optical bench
SPIRE FPU integration on the optical bench - Credits RAL
Cooler integration to SPIRE
Cooler integration to SPIRE - Credits RAL

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SPIRE instrument

SPIRE instrument (Spectral and Photometric Imaging REceiver) is built at Rutherford Appleton Laboratory (RAL) by a consortium led by M. Griffin, University of Wales, Cardiff, UK. It is composed of two parts:

    An imaging photometer with "spider-web" bolometer arrays at 0.3 mK with a field of view of 4'x8'
  Spire photometer side view Spire photometer side view
Credits RAL
Photometer side view
    A Fourier Transform Spectrometer with "spider-web" bolometer arrays at 0.3 mK with a field of view of 2.6'x2.6'
  Spire spectrometer side view Spire spectrometer side view
Credits RAL
Spectrometer side view

The french participation to SPIRE instrument SPIRE is done through two laboratories: the CEA/DAPNIA and the LAM.

The CEA/DAPNIA participation to the development consists in the realisation of the DRCU: warm unit (WU) composed of four sub-units in two boxes:

    DCU box which drives the photometer and the spectrometer detectors
    FCU box which consists in:
      the MCU which drives the "SMECm" and "BSMm" mecanisms of the focal plane;
      the SCU to manage the Thermal / Cooler / Calibration sub-systems;
      the PSU which supply power to the sub-systems.

The LAM participation to the SPIRE development consists in:

    the realisation of the FTS spectrometer mechanism, named SMECm
FTS mechanism of the SPIRE instrument
Credits CNRS/LAM/CNES
    the realisation of the MCU electronic to drive the mechanisms
    the realisation of the spectrometer and the photometer optics (Mirrors + Alignments)
SPIRE instrument mirrors
Credits CNRS/LAM/CNES
 

Latest update 04/06/2007