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The SWS90-SWS98 were short sequences of
commands for activation, de-activation and routine monitoring of the
instrument, under direct control of the instrument operators. They are
of little interest for observers but are included here for completeness.
They were:
- SWS90: SWS switch-on and complete RAM load. Leave the detector biases
switched off.
- SWS91: Try and cure the detectors by heating the detector substrates to the
maximum values (for this purpose electrical heaters were glued on the
substrates).
- SWS92: Switch on the detector biases, put the instrument in its default
operational state.
- SWS93: Try and cure the detectors by irradiating them with photons from the
`flashers'. For bands 2-6 this would have had no effect without the bias
switched on.
- SWS94: After the instrument has stabilised, or at any other moment, take a
dark current measurement and then return the instrument to its default
operational state. Introduced at the end of January 1996.
- SWS95: SWS post-helium band 1 detector setup sequence.
- SWS96: SWS post-helium band 1 internal wavelength calibration sequence.
- SWS97: SWS post-helium band 1 internal grating calibration sequence.
- SWS98: Switch off.
- SWS99: Reserved for the CUS/post-helium.
At the start of a revolution SWS90 to SWS94 were executed in sequence to
set the instrument up. SWS98 de-activated the SWS at the end of a
revolution. For the post-helium revolutions SWS95 to SWS97 were used to
activate the instrument, with SWS98 still used for de-activation.
Next: 4. Wavelength Calibration and
Up: 3. Instrument Observing Modes
Previous: 3.7 SWS99 - Post-Helium
ISO Handbook Volume V (SWS), Version 2.0.1, SAI/2000-008/Dc