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The interferometer consists of :
- Five antennas, each controlled by a VME-based microprocessor,
- One off-axis optical telescope per antenna, for pointing,
- Two (4 on the long term, 2 simultaneous IF) receivers per antenna,
- Continuum detectors for each receiver and each antenna, read
by a simple ADC by the ``phaser'' microprocessor.
- A 8-unit flexible correlator
- An HP-J200 computer named BURE1 for real-time command and
acquisition,
- A dedicated Ethernet link between BURE1 and the correlator units.
- An HP-J200 computer named BURE2 for data reduction, with
NFS mounted disks from the acquisition computer.
- A general Ethernet link between BURE1, BURE2, the antenna and
receiver microprocessors, terminals, etc...
- Many cables : low and high quality for the IF transmission, twisted
pairs for specific signals, etc...
The instrument may be used in several basic modes: OPTICAL pointing,
INTERFEROMETER observing, or TEST mode.
In addition, within the OBS program,
there is a CONFIGURE mode, which is used to specify and modify
the array configuration parameters.
Optical pointing is done essentially to check the mechanical behaviour
of the antennas. This is a very limited mode, with little associated software
and it is seldom used.
Next: Interferometer Backends
Up: OBS Users Guide IRAM
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Gildas manager
2002-02-04