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The instrument used in this calibration will have
- At At least four channels based on "classic" AXUV photodiodes (manufactured before Raj Korde sold the company)
- Quad diode for alignment
- Lyman alpha filter (121.1 nm) - the source of this filter will have to be determined
130
nm filternm filter
476 nm Interference filter to match previous calibrations
- Double Metal filters – Al, Be, Zr (holes). Al filters should have a protective layer of carbon on both sides
- Apertures
- On-board preamplifiers
Need to work out the interface between the instrument and the MLS data computer
- Serial link like XRS has now
- Current output
- counts output
The characterization of the instrument will be based on measurements with both monochromatic and undispersed synchrotron radiation.
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