1 / 24

Carbon Fibre Hexapod (Denmark)

The Mid-Infrared Instrument (MIRI) Medium Resolution Spectrometer for JWST Martyn Wells MIRI EC & UKATC. Spectrometer Pre Optics UKATC. Spectrometer Main Optics Netherlands. Deck (Leicester). Spectrometer Focal Plane Module (USA). Carbon Fibre Hexapod (Denmark). Imager (France).

halen
Download Presentation

Carbon Fibre Hexapod (Denmark)

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. The Mid-Infrared Instrument (MIRI) Medium Resolution Spectrometer for JWST Martyn WellsMIRI EC & UKATC

  2. Spectrometer Pre Optics UKATC Spectrometer Main Optics Netherlands Deck (Leicester) Spectrometer Focal Plane Module (USA) Carbon Fibre Hexapod (Denmark) Imager (France) Input Optics and Calibration Unit (Belgium)

  3. Summary description

  4. SPO SMO Spectrometer block diagram

  5. Spectrometer fov

  6. Exposure C Exposure B Exposure A Dichroic passbands

  7. Spectrometer – l ranges, R, sampling and fov

  8. Ray-trace diagram of the Channel 1 IFU

  9. Diagram of the output slit

  10. Integral Field Unit Optical Layout Spectrometer Pre-Optics

  11. 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

  12. 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.

  13. The light is dispersed by the grating. Dispersion direction

  14. ...and heads back to a fold mirror.

  15. ...which sends it to the final, camera mirror, which is a common optical element for Channels 1 and 2 (as is the fold mirror)

  16. The camera mirror forms the final image...

  17. ...on the Focal Plane Module (FPM), shown here as the green cylinder.

  18. Here comes the beam from the Channel 1 IFU, collimated and sent to one of Channel 1’s 3 gratings...

  19. ...where it is dispersed...

  20. ...and sent via this fold mirror to share the last two mirrors on its way to the FPM with the spectrum from Channel 2.

  21. Channel 2a spectra Constant wavelength positions

  22. Some manufactured components

More Related