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Why Stray-light in optical instruments matters and what to do about it

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Academic year: 2021

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Why stray-light in optical instruments matters

and what to do about it?

L. Clermont Centre Spatial de Liège

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Added values from space activities are crucial (earth observation, science, etc.)

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Optics is at the core of space instruments Optics Another lesser field A lesser field An even worst lesser field

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Optical designers build optical instruments by finding a configuration of optical elements which minimizes aberrations Optical elements (lenses, mirrors, diffractive elements) can bend rays to form an image

F F

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Minimizing aberrations is great …

but that’s not the only driver of optical performance

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Stray-light is light reaching the detector by following different paths or processes than the nominal beam

16:58:41

New lens from CVMACRO:cvnewlens.seq Scale: 0.56 05-Dec-17

XZ 44.64 MM 13:36:06 2 6 7 8 9 10 11 12 13 14 15 16 17 19

Ghost Trace for Surface Pair S12 - S8 06-Dec-17 52.57 MM

Nominal rays sequence

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- Broadening of the point spread function (PSF) - Addition of unwanted features on the detector - Decrease of the signal to noise ratio (SNR)

- Saturation of the detector Stray-light decreases the image quality

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The ingredients of stray-light: Source of light External source Thermal self-emission Fluorescence Non-nominal process Ghost reflection Scattering Diffraction Rogue paths Nominal process Stray-light

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Nomex fibers sticking out of the sun shield

Rogue rays from edge of sun shield can enter

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What to do against stray-light?

Design the instrument against stray-light (control) Predict the origin and level of stray-light (analysis) Verify the prediction experimentally (measurement)

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The stray-light engineering process is iterative and works as a feedback loop, it must consider also other aspects than optics

Optical design

Efficient against aberrations

System design

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Experimental characterization requires dedicated facilities

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Stray-light requirements are always more stringent Hardware optimization is not enough !

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For METOP-3MI, we have developed a stray-light correction algorithm, which works together with an on-ground

stray-light characterization

3D view of the payload

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What to remember?

Stray-light = critical concern (performance driver)

Need to be considered from early phase of mission @system level Hardware is the first cure, post-processing is the second

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