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Draft agenda

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Draft agenda. STEAM overall status. Science objectives. Present mission concept ... wedged slit to equalise signal levels (or internal scan). Based on OSIRIS. ... – PowerPoint PPT presentation

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Title: Draft agenda


1
Draft agenda
  • STEAM overall status
  • Science objectives
  • Present mission concept
  • Reports by participants
  • Study activities and future meetings.
  • Instrument requirements
  • International collaboration
  • Other

2
The STEAM spacecraft
  • Launch on Start-1
  • Ascending node at 600 or 900
  • Circular, polar 700 km sun-sync orbit
  • 4 year lifetime
  • Control and down-link to ESRANGE
  • 3-axis stabilised using reaction wheels
  • Rear viewing star trackers, sun sensors
  • 1 arc minute pitch control accuracy
  • 160 kg (54 kg payload)
  • 277 W average power

3
STEAM Imaging Radiometer
  • Imaging with 8 beams to support tomographic 3-d
    retrievals.
  • Improved sensitivity and horizontal resolution,
    no gaps in coverage due to scanning.
  • Results in 2 km altitude by 40 km along-track
    grid.
  • H2O, O3, and CO in the upper troposphere / lower
    Stratosphere (UT/LS), 5 to 28 km (the 340 GHz
    band).
  • O3, N2O, H2O and ClO in the Stratosphere, 15 to
    40 km (the 500 GHz band).
  • LO 337.9, IF 5.9-13.9, LSB/USB 324.0-332.0/
    343.8-351.8 GHz
  • LO 496.25, IF2.75-6.75, LSB/USB 489.5-493.5/
    499-503 GHz

4
STEAM Radiometer antenna
  • Designed, built and tested as Odin.
  • CFRP face-sheets on honeycomb.
  • Vacuum deposited aluminium.
  • 15 micron RMS surface (Odin was 8).
  • Simple box-like CFRP support structure.
  • Integrates star tracker optical heads and
    receiver front-end parts.
  • Back side radiatively coupled to spacecraft.

5
STEAM Radiometer
6
STEAM optics
  • One optical axis
  • 4 beam building block
  • 4 beams in each polarisation, when combined
    overlap at half-power width.
  • One redundant drive switch mechanism, calibrating
    one polarisation at a time.
  • Few armin nodding motion by spacecraft to fill in
    gaps.

7
STEAM mixers and LO
  • Sub-harmonically pumped, planar mixer chips (self
    biased) for both frequency bands.
  • LO coupled via waveguide and integrated frequency
    multipliers.
  • LO generated either from Gunn sources or low
    frequency source followed by multipliers and
    power amplifiers.
  • Standard hybrid mode horns or simplified design.

8
STEAM spectrometers
  • Chip set (9x16mm) tested at 1.7 GHz
  • Flight production at 2 GHz per chip
  • Power down of unused lags (1024)
  • Possibility to go to 4 GHz per chip with more
    time multiplex and 0.18 micron process.

9
STEAM optical instrument
  • Range 400 800 or 1000 nm.
  • 30 km height range.
  • wedged slit to equalise signal levels (or
    internal scan).
  • Based on OSIRIS.
  • Canadian contribution.
  • This study assumed OSIRIS properties.

10
STEAM study result
  • Relatively well defined.
  • Smaller than Odin and much simplified both
    payload and attitude control.
  • Substantial (as Odin) payload power. Huge
    technical leap utilised to implement multi-beam
    (16) receivers and large (8 GHz) bandwidth.
  • Clearly feasible.
  • Payload should be pre-developed (prototype)
  • 300 MSEK including 2 years operation
  • Swedish-French-Canadian-?
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