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FRAUNHOFER INSTITUTE FOR APPLIED OPTICS AND PRECISION ENGINEERING IOF ASPHERICAL MIRRORS FOR ASTRONOMY AND SPACE 1 Optical assembly of the athermal IR-spectrometer MERTIS. 2 F reeform mirror with precise reference elements in the interferometric setup com- prising a CGH. 3 MRF processing of an aspheric aluminum mirror with amorphous NiP coating. Motivation Aspheres and optical freeforms are more and more important applications for space and astronomy. Mirror based telescopes are suitable for multi spectral imaging in the range from IR to UV; applications in the VIS or UV spectral range require an ultra-smooth surface in terms of figure and roughness. Technologies Ultra-precision machining with diamond tools, in combination with polishing and figuring techniques, enables the manu- facturing of high quality mirrors with various surface shapes in space certified materials. Highly sensitive interferometric metrology using Computer Generated Holograms (CGH) or tactile measurement techniques allows correction cycles to reduce form errors. For applications in the VIS or UV spectral range, post-polishing and post-figuring processes like ion beam figuring (IBF) and magneto rheological finishing (MRF) are applied on an amor- phous nickel-phosphorous (NiP) coating on the CTE-matched mirror substrate. Additionally, reflection and protection layers can be deposited. Results Aspherical mirror (190 mm x 250 mm) - Al-6061, NiP-coated, protected Ag - SPDT, post-polishing, IBF-figuring - Micro roughness (WLI 50x): < 1 nm (rms) - Shape irregularity: < 14 nm (rms); 110 nm (p-v) Freeform mirror (Ø 320 mm) - AlSi-alloy, NiP-coated - SPDT, MRF-figuring, post-polishing - Micro roughness (WLI 50x): < 3 nm (rms) after MRF < 0.8 nm (rms) after polishing - Shape irregularity: < 16 nm (rms); 120 nm (p-v) Fraunhofer Institute for Applied Optics and Precision Engineering IOF Albert-Einstein-Straße 7 07745 Jena, Germany Director Prof. Dr. Andreas Tünnermann Department Precision Engineering Head of Department Dr. Ramona Eberhardt Contact Andreas Gebhardt Phone +49 3641 807-340 [email protected] www.iof.fraunhofer.de 2 3 1
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ASPHERICAL MIRRORS FOR ASTRONOMY AND SPACE · ASTRONOMY AND SPACE 1 Optical assembly of the athermal IR-spectrometer MERTIS. 2 Freeform mirror with precise reference elements in the

Mar 29, 2021

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Page 1: ASPHERICAL MIRRORS FOR ASTRONOMY AND SPACE · ASTRONOMY AND SPACE 1 Optical assembly of the athermal IR-spectrometer MERTIS. 2 Freeform mirror with precise reference elements in the

F R A U N H O F E R I N S T I T U T E F O R A P P L I E D O P T I C S A N D P R E C I S I O N E N G I N E E R I N G I O F

ASPHERICAL MIRRORS FORASTRONOMY AND SPACE

1 Optical assembly of the athermal

IR-spectrometer MERTIS.

2 F reeform mirror with precise reference

elements in the interferometric setup com-

prising a CGH.

3 MRF processing of an aspheric aluminum

mirror with amorphous NiP coating. Motivation

Aspheres and optical freeforms are more

and more important applications for space

and astronomy. Mirror based telescopes are

suitable for multi spectral imaging in the

range from IR to UV; applications in

the VIS or UV spectral range require an

ultra-smooth surface in terms of fi gure and

roughness.

Technologies

Ultra-precision machining with diamond

tools, in combination with polishing and

fi guring techniques, enables the manu-

facturing of high quality mirrors with

various surface shapes in space certifi ed

materials. Highly sensitive interferometric

metrology using Computer Generated

Holograms (CGH) or tactile measurement

techniques allows correction cycles to

reduce form errors. For applications in the

VIS or UV spectral range, post-polishing

and post-fi guring processes like ion beam

fi guring (IBF) and magneto rheological

fi nishing (MRF) are applied on an amor-

phous nickel-phosphorous (NiP) coating

on the CTE-matched mirror substrate.

Additionally, refl ection and protection

layers can be deposited.

Results

Aspherical mirror (190 mm x 250 mm)

- Al-6061, NiP-coated, protected Ag

- SPDT, post-polishing, IBF-fi guring

- Micro roughness (WLI 50x):

< 1 nm (rms)

- Shape irregularity:

< 14 nm (rms); 110 nm (p-v)

Freeform mirror (Ø 320 mm)

- AlSi-alloy, NiP-coated

- SPDT, MRF-fi guring, post-polishing

- Micro roughness (WLI 50x):

< 3 nm (rms) after MRF

< 0.8 nm (rms) after polishing

- Shape irregularity:

< 16 nm (rms); 120 nm (p-v)

Fraunhofer Institute for Applied

Optics and Precision Engineering IOF

Albert-Einstein-Straße 7

07745 Jena, Germany

Director

Prof. Dr. Andreas Tünnermann

Department Precision Engineering

Head of Department

Dr. Ramona Eberhardt

Contact

Andreas Gebhardt

Phone +49 3641 807-340

[email protected]

www.iof.fraunhofer.de

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