After seeing this, Dana used his Zemax model to evaluate the focus for different wavelengths and positions. Here is what he came up with (NFP = Nominal Focus Position, units are µm):
Telescope separation
|
IRTF focus position delta
|
Entrance focus position delta
|
Slit focus position delta
|
7micron Beam size at slit
|
7micron Airy disk at slit
|
7micron Beam size at detector
|
7micron Airy disk at detector
|
12micron Beam size at slit
|
12micron Airy disk at slit
|
|
7021.096
|
-20000
|
-8535
|
-3936
|
368
|
174
|
430
|
174
|
300
|
298
|
|
7021.048
|
-10000
|
-6545
|
-3025
|
292
|
174
|
336
|
174
|
222
|
298
|
|
NFP
|
7021.012
|
-1764
|
-5116
|
-2475
|
236
|
174
|
266
|
174
|
165
|
298
|
7020.960
|
10000
|
-3000
|
-1700
|
150
|
174
|
164
|
174
|
82
|
298
|
|
7020.916
|
20000
|
-1290
|
-872
|
86
|
174
|
91
|
174
|
16
|
298
|
|
7020.872
|
30000
|
534
|
-122
|
28
|
174
|
74
|
174
|
60
|
298
|
|
7020.820
|
40000
|
2856
|
732
|
65
|
174
|
142
|
174
|
142
|
298
|
|
7020.784
|
50000
|
3852
|
1340
|
122
|
174
|
200
|
174
|
200
|
298
|
|
7020.736
|
60000
|
5795
|
2131
|
197
|
174
|
284
|
174
|
277
|
298
|
We're running at 5µm, and Dana designed the system for 12µm light. His 7µm data point shows best focus for 7µm is 32mm away from the design focus, so our finding of a ~40µm difference at 5µm isn't absurd.
Having found this out, we decided to run a focus check in camera mode (knowing the dubious character of the alignment mirror) to see whether we might be fooling ourselves. Here is what the spot looks like as we run the blackbody source over a90mm range along the Z-axis:
In this movie the BB is moved along Z toward the entrance window at 10mm/frame. The two spots may be coalescing (or simply passing one another) as we get closer to the entrance window, but it's difficult to be quantitative. This data is stored on the mac mini as 'Camera Mode BB Focus Run' if anyone wants to look at it more closely.


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