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Op#cs & Instruments Lecture 8: Op#cal Design Christoph U. Keller

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Page 1: Opcs & Instruments - Leiden Universityhome.strw.leidenuniv.nl/~keller/Teaching/OAI_2015/OAI_2015_L08...• can be sketched on paper or in a spreadsheet ... r2 92.6792 0.02 -1.09657

Op#cs&InstrumentsLecture8:Op#calDesign

ChristophU.Keller

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Overview•  Introduc4on•  Requirements•  Op4calDesignPrinciples•  Ray-TracingandDesignAnalysis•  Op4miza4onandMeritFunc4on•  ToleranceAnalysisandOptomechanicalDesign•  WavefrontErrorBudget•  TransmissionBudget

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 2

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Introduc#on

•  op4caldesignisnotlinear,butitera4veprocess•  closecouplingbetweenop4cal,mechanical,electrical,controls,soLwaredesignandscience

•  op4caldesignisfirstdesigneffort,providesfirstideaofhowfinalinstrumentwilllook

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 3

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TypicalRequirements•  spa4alrange:field-of-view(FoV)•  spa4alresolu4on,spa4alsampling•  spectralrange&resolu4on,sampling•  transmission•  detectorpixelsize•  stabilityandrepeatability•  polarimetricsensi4vityandaccuracy

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 4

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ExampleOp#calDesignRequirements

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 5

Parameter Specification CommentSpectralspectral lines 630.1515, 630.2507 nm,

854.2089 nm, 1083.0 nmselected suitable spectral lines

spectral resolution 200,000wavelength range 630.1515-0.05 nm to

630.2507+0.05 nm854.2 +/- 0.1 nm1083.0 +/- 0.5 nm

were unable to design efficient instrumentover full range of 600 to 1600 nm

spectral lines at least two simultaneouslyPolarimetrytype 630.2 nm: I,Q,U,V

854.2 nm: I,V1083.0 nm: I

Analysis of vector polarimetry in 854.2 nmnot clear, traded wider spectral range in1083.0 nm for polarimetry

sensitivity 0.0002 per pixel in 0.5 srelative accuracy 0.001Miscellaneousimage motion stabilization at about 100 Hz to improve spatial resolutioncloud detection at user-specified

levelreal time seeing monitoring for information onlyinterruption of scanning during

continuation after clouds

excerpt from SOLIS VSM Optical Design Requirements

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BoundaryCondi#ons•  sitecharacteris4cs(seeing,temperatures)•  telescopeproper4es•  telescopeinterfaces•  instrumentloca4on(fixedorvariablegravityvector,spaceandweightlimits)

•  detectoravailability•  available€,$,...

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 6

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RequirementsReview•  requirementsreview

–  iden4fiesunnecessary,incompa4bleandomiXedrequirements

– ensuresthatallrequirementscanbeverifiedandtracedbacktoscien4ficneeds

•  op4caldesignrequirements– derivefromsciencerequirements– setboundarycondi4onsforop4caldesignintermsofop4calquan44es

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 7

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Op#calDesignPrinciples1-31.  Minimizethenumberofop4calcomponents

–  addi4onalelementsaddcost,ghosts,scaXeredlight–  but:addi4onalelementsincreaseperformance

2.  Minimizetheradiiofcurvature–  reducesaberra4ons–  easesmanufacturingandalignment–  but:mightrequiremoreelementsandlongdesigns

3.  Maximizetheallowedtolerances–  simplifiesmanufacturing,mechanicaldesignand

opera4onalrequirements

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 8

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Op#calDesignPrinciples3-63.  Placecomponentsclosetofocusifthey

introducewavefrontaberra4ons4.  Placecomponentsclosetopupilifallfield

pointsmustpasssamepartofcomponent5.  Placecomponentsincollimatedbeamifallrays

fromonefieldpointshouldpassthecomponentunderthesameinclina4onangle

6.  Placecomponentsinatelecentricbeamifthecomponentissensi4vetotheinclina4onangle

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 9

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Example:FilterinImage

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 10

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Example:FilterinPupil

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 11

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Example:FilterinTelecentricBeam

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 12

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Op#calDesignPrinciple77.  Oversizeop4calelements

–  op4calmanufacturingqualityalwaysworseatedge

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 13

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Global Design Choices •  lenses or mirrors (depends on wavelength range) •  choice of dispersing elements (prism, grating) •  location of aperture stop •  locations of image and pupil planes •  sampling (Nyquist: >2 pixels per resolution element) •  (dichroic) beam-splitting •  (de-)magnification •  F-numbers (problems ~1/F-number) •  collimated beam? •  telecentric beam?

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 14

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First-OrderDesign•  first-orderop4caldesignsuse

–  idealop4calelements(e.g.paraxialsurfaces)– centralandextremefieldpointsandrays–  imageandpupilloca4ons

•  establishesgeneralconfigura4on•  oLenbasedonexis4ngdesigns•  canbesketchedonpaperorinaspreadsheet•  providefirstideaofsizeofdifferentdesigns

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 15

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Example First-Order Design 1

•  m=f2/f1 •  minimum geometrical aberrations for

symmetric system (m=1)

f1 f2 f2

“Offner relay”

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 16

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ExampleFirst-OrderDesign2

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 17

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First-Order Design Example 3

EPICS-EPOL

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 18

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First-Order Design Example 4

SPICES

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 19

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Collimated vs. Converging Beam •  components in collimated beam?

–  dispersion element –  cold stop –  Lyot stop –  filter? –  polarization modulator?

•  components in converging beam? –  slit –  coronagraphic mask –  detector –  filter?

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 20

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Ray Tracing •  Ray-tracing based on geometrical optics

approximation (wavefronts are locally flat) •  Rays are traced from source to image •  Sequential ray-tracing traces rays according to

predetermined sequence of optical elements •  Non-sequential ray-tracing determines at each step

next surface a given ray will reach (much slower) •  Optical design programs: WinLens, ZEMAX, OSLO •  Programs only useful once major design decisions

have already been made!

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 21

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Ray Tracing Software (sequential)

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 22

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Spot Diagrams

Jan

Apr Jul

custom spherical doublets

S5T

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 23

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Aberration Plots •  optical path differences •  Seidel diagram

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 24

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Op#miza#on•  builtintomostop4caldesignsoLware•  automa4callyimprovesperformance•  degreesoffreedom=variablesofop4caldesign

–  radiiofcurvatureofop4calsurfaces– spacingbetweenelements– conicconstants– glassthicknesses

•  canchangeglasstype•  generallydoesnotaddorremoveop4cs

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 25

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Op#miza#on:MeritFunc#on•  meritfunc4on

– basedondesignrequirements– designop4mal=meritfunc4onatglobalminimum

•  meritfunc4ondependson– op4caldesignparameters(restric4onsondiameters,thicknesses,etc.)

– systemparameters(f-numbertobeachieved,overallsystemlength,etc.)

– aberra4onparameters(suchasrmswavefrontaberra4on,fieldcurvatureetc.,oLenasafunc4onoffieldangleandwavelength)

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 26

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Design Example 1: SOLIS VSM

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 27

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Design Example 2: X-shooter

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 28

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Design Example 2: X-shooter

simulated from optical design measured

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 29

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ToleranceAnalysis•  determinestolerancestowhich

– op4calelementshavetobemanufactured– op4calelementshavetobeposi4oned– environmentalparametershavetobecontrolled

•  needstoconsideralldesignparametersthataresubjecttoerrors

•  differentop4caldesignsmayhavesameperformancebutonemaybemuchmoredemandingonthemanufacturingand/oralignmentthananotherdesign

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 30

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Sensi#vityAnalysis•  toleranceanalysisbasedonmeritfunc4on

– maybethesameasusedforop4miza4on

•  sensi4vityanalysis– simplestformoftoleranceanalysis–  revealssensi4vityofmeritfunc4onwithrespecttoanassumederrorineachdesignparameter(e.g.knownmanufacturingtolerances)

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 31

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InverseSensi#vityAnalysis•  inversesensi4vityanalysis

– determinesmaximumallowederrorindesignparameterforgivenmaximumallowedchangeinmeritfunc4on

– providesfirstapproxima4ontotolerancestobespecified

– doesnotconsidercoupledeffectofsimultaneouserrorsinalldesignparameters

•  MonteCarlotoleranceanalysisprovidesrealis4ces4mateofexpectedperformancebyusingsta4s4caldistribu4ons

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 32

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Tolerancing Example

1. The parameters of the mirror under testing (the units of length are in mm): Radius 1600 ±2CC -1.09638617 ±0.002Clear aperture 528Testing Aperture 536

2. The optical perameters of the null lens testing system

Radius Thickness Glass Diameter ConicPoint source 280 mm Null lens 69.5879 mm 12 BK7 64 mm

plane 169.082 mm Field lens 92.6792 mm 5 mm BK7 16 mm

plane 53.994 mm Curverture center 1600 mm Mirror under tesitng -1600 mm Mirror 536 -1.096386

3. Null lens tolerance

Radius tolerance Thickness tolerance TIR* irigularity(pv)Point source 280 0.04Null lens 69.5879 0.02 12 0.01 0.01 0.1

plane 169.082 0.03 0.1Field lens 92.6792 0.02 5 0.02 0.005 0.125

plane 53.994 2 0.1251600

Primary mirror -1600 Total irigularity .127

*TIR: Total indicator runout

Toerance sensitive analysis tableerrors CC Δ CC R Δ R budget error CC errors

r1 69.5879 0.02 -1.09576 .00062 1599.9329 -0.0671 0.02 0.000624-0.02 -1.09701 -.00063 1600.0673 0.06732

r2 92.6792 0.02 -1.09657 -.00018 1599.9967 -0.003262 0.02 -0.000183-0.02 -1.09620 .00018 1600.0033 0.00326

d1 280 0.02 -1.09576 .00062 1600.0804 0.08041 0.04 0.0012482-0.02 -1.09701 -.00063 1599.9195 -0.0805

d2 12 0.03 -1.09738 -.00099 1599.9283 -0.0717 0.01 -0.000331-0.03 -1.09665 -.00026 1599.9106 -0.0894

d3 169.082 0.05 -1.09732 -.00094 1600.0224 0.02238 0.03 -0.000561-0.05 -1.09545 .00093 1599.9776 -0.0224

d4 5 0.02 -1.09637 .00001 1600.0132 0.0132 0.02 1.309E-05-0.02 -1.09640 -.00001 1599.9868 -0.0132

d5* 53.994 1 -1.09572 .00067 1600.9999 0.9999 2 0.0013325-1 -1.09705 -.00067 1599.0001 -0.9999

Total conic constant error 0.0020447

*The error of d5 including the radius measurement error of the primary mirror.

Element

required tolerance

Element

excerpt from SOLIS VSM conic constant tolerance analysis

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 33

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DrawingExample

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 34

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System Budgets •  Look at the whole instrument at once •  Find the optimum balance •  The whole is the sum of its parts •  Examples:

– wavefront error –  transmission/photon budget –  thermal background – polarimetric accuracy – weight, cost, ...

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 35

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Wavefront Error Budget

sensitivities from ZEMAX:

overall:

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 36

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Photon Budget Quantity wavelength (nm) units comment

630.2 854.2 1083

Total transmission 0.228804 0.227108 0.225067 unpolarized

Photoelectric flux 1.23E+08 1.12E+08 3.13E+06 e-/s per pixel

CCD maximum detection 1.20E+08 1.20E+08 6.00E+07 e-/s given by full-well depthDetected flux 1.20E+08 1.12E+08 3.13E+06 e-/s

Stokes Q modulation efficiency 0.58Stokes V modulation efficiency 0.50 1.00Stokes I noise in 0.5s 1.29E-04 1.34E-04 7.99E-04Stokes Q,U noise in 0.5s 2.24E-04Stokes V noise in 0.5s 2.58E-04 1.34E-04

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 37

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Transmission Budget

X-shooter

Christoph U. Keller, [email protected] Optics & Instruments: Lecture 8, Optical Design 38