the mid-infrared instrument (miri) medium resolution spectrometer for jwst martyn wells miri ec...
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The Mid-Infrared Instrument (MIRI)
Medium Resolution Spectrometer for JWST
Martyn WellsMIRI EC & UKATC
Carbon Fibre Hexapod (Denmark)
Spectrometer Main OpticsNetherlands
Imager (France)
Input Optics and Calibration Unit
(Belgium)
Deck (Leicester)
Spectrometer Focal Plane
Module (USA)
Spectrometer Pre Optics
UKATC
Summary description
Spectrometer block diagram
IFU 1
IFU 2
IFU 3
IFU 4
Collimator
Collimator
Collimator
Collimator
Camera 1
Camera 2
FPA 1
FPA 2
Grating
Grating
Grating
Grating
Dichroic 1
Dichroic 2
Dichroic 3
SPO SMO
Spectrometer fov
-4
-3
-2
-1
0
1
2
3
4
-4 -2 0 2 4Field of view across slices (arcsec)
Fie
ld o
f vie
w a
lon
g s
lices (
arc
sec)
IFU 1
IFU 2
IFU 3
IFU 4
Dichroic passbands
1
1. 2
1. 4
0 5
10 15 20 25 30
Channel 1A Channel 1B Channel 1C
Channel 2A Channel 2B Channel 2C
Channel 3A Channel 3B Channel 3C
Channel 4A Channel 4B Channel 4C
Exposure A
Exposure B
Exposure C
Spectrometer – ranges, R, sampling and fov
WHEEL A
WHEEL B
CHANNEL 1 APO
CHANNEL 2 APO
INPUT MIRROR
Blocking filter
Light trap
Fold mirror
Adjustable fold mirror
CHANNEL 3 exit port
D1
D2
D3
Light trap
Ray-trace diagram of the Channel 1 IFU
David Lee 17 February 2004
Image Slicer MirrorRe-imaging mirrors
Output slits
Location of input Pupil
IFU input fold mirror
Location of output Pupils
~150 (length varies with slice position)Slice #1 151.60 mm z offset = 2.32 mmSlice #11 149.28 mm z offset = 0.00 mm
10 31.1
22.1
41.3
Channel 1 - IFU APO exit fold mirror
Diagram of the output slit
Integral Field Unit Optical Layout
M1
M2M4
M3APO output fold
Image slicer mirror
Roof mirror
Re-imaging mirror array
Outputslitets
Pupilimages
INPUT Spectrometer Pre-Optics
Here are the flattened envelopes of the sliced and stacked sky images, heading off to the spectrometer collimator mirrors in the Spectrometer Main Optics (SMO)
The position of the Channel 2 collimator mirror
Here, the beam from the Channel 2 collimator is shown, heading back to one of Channel 2’s three diffraction gratings.
The position of a Channel 2 grating.
The light is dispersed by the grating.
Dispersion direction
...and heads back to a fold mirror.
...which sends it to the final, camera mirror, which is a common optical element for Channels 1 and 2 (as is the fold mirror)
The camera mirror forms the final image...
...on the Focal Plane Module (FPM), shown here as the green cylinder.
Here comes the beam from the Channel 1 IFU, collimated and sent to one of Channel 1’s 3 gratings...
...where it is dispersed...
...and sent via this fold mirror to share the last two mirrors on its way to the FPM with the spectrum from Channel 2.
Channel 2a spectra
Constant wavelengthpositions
Some manufactured components