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    ESA > Our Activities > Observing the Earth > The Living Planet Programme > Earth Explorers > SMOS

    SMOS measurement principle

    SMOS mission overview

    For optimum results, SMOS will measure microwave radiation emitted from Earth's surface within the L-band (1.4 GHz) using an interferometric radiometer.

    Measurement principles

    Moisture and salinity decrease the emissivity of soil and seawater respectively, and thereby affect microwave radiation emitted from the surface of the Earth. Interferometry measures the phase difference between electromagnetic waves at two or more receivers, which are a known distance apart – the baseline.

    Interferometry principle
    Interferometry principle

    The SMOS radiometer will exploit the interferometry principle, which by way of 69 small receivers will measure the phase difference of incident radiation. The technique is based on cross-correlation of observations from all possible combinations of receiver pairs. A two-dimensional 'measurement image' is taken every 1.2 seconds. As the satellite moves along its orbital path each observed area is seen under various viewing angles.

    From an altitude of around 758 km, the antenna will view an area of almost 3000 km in diameter. However, due to the interferometry principle and the Y-shaped antenna, the field of view is limited to a hexagon-like shape about 1000 km across called the 'alias-free zone'. This area corresponds to observations where there is no ambiguity in the phase-difference.

    SMOS will achieve global coverage every three days.


    Mission approach

    Mission SMOS
    Launched 2 November 2009
    Duration Minimum 3 years
    Instrument Microwave Imaging Radiometer using Aperture Synthesis - MIRAS
    Instrument concept Passive microwave 2D-interferometer
    Frequency L-band (21 cm-1.4 GHz)
    Number of receivers 69
    Receiver spacing 0.875 lambda = 18.37 cm
    Polarisation H & V (polarimetric mode optional)
    Spatial resolution 35 km at centre of field of view
    Tilt angle 32.5 degrees
    Radiometric resolution 0.8 - 2.2 K
    Angular range 0-55 degrees
    Temporal resolution 3 days revisit at Equator
    Instrument data rate 89 kbps H & V pol.
    Mass Total 658 kg launch mass comprising: platform 275 kg, payload 355 kg, fuel 28 kg
    Orbit Sun-synchronous, dawn/dusk, quasi-circular orbit at altitude 758 km. 06.00 hrs local solar time at ascending node.
    Launcher Rockot, KM-Breeze upper stage
    Bus Proteus (1 m cube)
    Power Up to 1065 W (511 W available for payload; 78 AH Li-ion battery.
    Spacecraft Operations Control Centre CNES,Toulouse, France
    S-Band TTC link 4 kbps uplink, 722 kbps downlink
    Payload Mission and Data Centre ESAC, Villafranca, Spain
    X-Band data downlink 16.8 Mbps

    SMOS mission milestones

    June 2004
    Start of payload construction Phases C/D

    April 2004
    First joint SMOS/Aquarius/Hydros Workshop held in Miami, USA

    November 2003
    Approval for full implemention

    October 2003
    End of payload Phase B, design completed

    April 2003
    Fourth SMOS Workshop held in Porto, Portugal

    November 2001
    End of payload Phase A with scientific and technical review. Recommendation received to proceed with implementation.

    December 2001
    Third SMOS Workshop held in Oberpfaffenhofen, Germany

    November 2000
    Second SMOS Workshop held in Toulouse, France

    October 2000
    Start of payload feasibility studies (Phase A)

    September 1999
    First SMOS Workshop held in Barcelona, Spain

    April 1999
    Selection of SMOS

    July 1998
    Call for proposals

    Last update: 2 November 2009

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