Payload Module configuration
The Payload Module (PLM) is the main supporting structure for the complement of instruments and various deployable features. The internal design of the PLM allows these instruments to work optimally.
An overview of what the integrated PLM provides:
The PLM has a 'box' shape structure with a central cylinder as the main structural load path to the Service Module (SVM). It houses the payload instruments (see relevant article 'instrument summary') and the payload support systems. Instrument sensors and antennas are mounted on the external panels, while most of the electronics units are accommodated inside the PLM.
Thermal control of the PLM is in charge of maintaining all electronics and instruments in predefined operational and non-operational temperature limits.
Measurement data acquisition, handling, and storage
Scientific data acquisition, formatting, encryption and storage. A dedicated unit is implemented to adapt the National Oceanic and Atmospheric Administration (NOAA) interfaces to European standards for the American instruments.
Each unit or instrument is powered through a switchable and protected line, provided by specific PLM units. Unregulated power is distributed to the European instruments while a dedicated unit is providing the American instruments with regulated 28 V power.
Command and control for the PLM elements
A dedicated data bus, based on the European On-Board Data Handling Standard (OBDH), is used by the PLM. The Payload Module Computer (PMC) receives commands from the SVM and interfaces with the European instruments Instrument Control Units (ICUs) and Microwave Humidity Sounder Protocol Conversion Unit (MPU), as well as with a specific PLM unit for the American instruments (NIU).
Measurement data transmission to ground
Involves the transmission to ground of Consultative Committee for Space Data Systems (CCSDS) packetised data through the High Resolution Picture Transmission (HRPT), Low Resolution Picture Transmission (LRPT) and X-band links.
PLM design considerations
The PLM external configuration is mainly driven by the fields of view and performances of instruments, sensors, radiators and antennas, as well as the available volume under launcher fairings.
The internal configuration has been driven by the following principles:
- provision of sufficient radiator area for heat dissipation of internal units (passive thermal control)
- modular grouping of PLM subsystems or functional units and instrument units to allow for pre-integration and testing on single panels
- minimal failure propagation to other instruments/subsystems in case of unsuccessful antenna deployment (e.g. only Advanced Scatterometer (ASCAT) units accommodated on the panels 'shadowed' by the stowed ASCAT antennas)
- optimal length for loss-sensitive cabling like antenna-receiver connections
- optimal harness routing in conjunction with modular assembly flexibility
The PLM accommodates various deployable elements:
- the solar array, which is fixed to the PLM zenith side only during launch. Its deployment is controlled solely by the SVM
- the GPS-based Atmospheric Sounder (GRAS) GAVA antenna is deployed by a spring mechanism which is released fully under SVM control
- the fore and aft ASCAT antenna assemblies, which are released by pyros from the SVM and further deployed under motor control from the PLM
- the Low Resolution Picture Transmission (LRPT) and Combined Receive Antenna (uplink) (CRA), similar to the ASCAT antennas, are both released by the SVM and subsequently further deployed under motor control from the PLM
Last update: 20 April 2006