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ODS, the Optical Depth Sensor
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General descriptions

Components:
  • Optical head : a system of 2 parabolic mirrors, focalizing the sky onton 1 photodiode, using 1 central mask to:
    • Obtain alternating FOV 25° - 50 °
    • Reduce specular scattering of dust cover on optical system
  • Electronics : 8-decade logarithmic amplification, converting photodiode current to output voltage, temperature compensated, to work with:
    • Both direct solar intensity and twilight intensity
    • Martian temperature variation from -120°C to 50°C

NETLANDER specifications

General specifications:
  • Number of channel : 2
  • Mass : 90g (25g×2 optical head + 20g×2 electronics, cables not included)
  • Comsomation : 30mW
  • Data rate : 2kb/day
Figure 1. Mechanical and optical layout of optical head of ODS in NETLANDER version of two channels: (1) upper parabolic mirror and entrance pupil, (2) lower parabolic mirror, (3) black wall, (4) black central mask, (5) silicon photodiode, (6) temperature sensor, (7) micro-porous pressure equalizer, (8) coaxial cables, (9) sunlight path.

Photodiode: Electronics:
  • Typical transfer function (CSVdata)
    Figure 2. Typical electronics transfer function, from photodiode current (A) to output voltage (V), with varying temperature (from -50°C to 50°C). Between range of -3V to 3V, the output is nearly linearly dependent on logarithm of current and independent with temperature; except for temperature as high as 50°C and low current (observation at night, rarely with temperature as high).

  • Typical inversed transfer function (CSVdata)

References

  • Maria, J.-L., Tran, T.T., Pommereau, J. P. et al., Technical aspects of the optical depth sensor, Advances in Space Research, accepted.
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