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hg [2021/11/24 23:55] mbroharthg [2024/02/08 18:23] (current) – external edit 127.0.0.1
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 The zenith prism rotates to the test lamps (position 0), the iris is opened, FW#1 is rotated to the quartz disk (position 1), FW#2 to ND=0 (position 0).\\  The zenith prism rotates to the test lamps (position 0), the iris is opened, FW#1 is rotated to the quartz disk (position 1), FW#2 to ND=0 (position 0).\\ 
  
-Following the initial set-up and lamp warm-up, the grating is scanned in the forward and reverse direction and the resulting combined spectrum is compared to a stored spectrum. Corrections to the micrometer position are made, and if the adjustment required is greater than 2 steps (.012nm) then the scan is repeated. A test for the presence of Hg lamp radiation is made prior to the beginning of the scan, and if it is not there, an FR test is done to reposition the micrometers to pre-set initialisation values and the test is redone.+Following the initial set-up and lamp warm-up, the grating is scanned in the forward and reverse direction and the resulting combined spectrum is compared to a stored spectrum. Corrections to the micrometer position are made, and if the adjustment required is greater than 2 steps (.012nm) then the scan is repeated. A test for the presence of Hg lamp radiation is made prior to the beginning of the scan, and if it is not there, an FR test is done to reposition the micrometers to pre-set initialization values and the test is redone.
  
 Refer to [[lamp|Lamps]] Refer to [[lamp|Lamps]]
  
hg.1637798119.txt.gz · Last modified: 2021/11/24 23:55 by mbrohart

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