mit2 71s09 gfinal sol
TRANSCRIPT
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 19
2710
Optics
Final
Exam
Solutions
Spring
lsquo09
1 Considerthefollowingsystem
(a)
If
we
position
an
on-axis
point
source
at
the
center
of
the
object
plane
(front
focal plane of L1) a collimated ray bundle will emerge to the right of L1 and
itsdiameter issetbyS1 thereforeS1istheaperturestop(AS) Similarly S2
limits the lateral extent of an imaged object (consider an off-axis point source)andthusitrsquosourfieldstop(FS)
(b) Theentrancepupilistheimageof theASbytheprecedingopticalcomponentsTofinditslocationweusetheimagingcondition
1 1 1 S of 1
2f 123
+ = S i = =
S o
S i
f 1
rArr
S o
minusf 1
f 1( 23
minus1)
2f 1S o =
S i =
minus2f 1 (virtual)3
rArr
Sotheentrancepupil is locatedat2f 1
totherightof L1 Tofind itsradiuswe
computethelateralmagnification
S iM L
=
minusS o
= 3
rarrrEnP
= 3a1
Fortheexitpupil(ExP)
f 1
( f 3
1 +f 2)f 2
f 22
S o
= +f 2 S i = =f 2
+3 (totherightof L2)
3
f 1
f 1+
f 23 f 2minus
+f 2)minus3f f
1
2( f 3
1
f 2
f 2M L
=( f 1 +f 2)
=
minus3
f 1
(inverted)
rarr rExP
= 3
f 1
a1
3
TheexitwindowisthesameasS2bull
The entrance window is the image of S2 through the preceding optical elebull
ments(ie combinationof L1andL2) Itisf 1
totheleftof L1
1
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 29
(c) Solution
Thenumericalapertureistanα
asympα
asympsinα
asympNA
asymp
a1
f 1
2X s
2f 1a2
2a2Thefieldof view(FOV)is FOV=2β = = =
3f 1
3f 1f 2
3f 2
(d)
The
location
of
S1
limits
the
FOV
because
of
the
requirement
for
the
CR
to
gothrough the center of the aperture stop (AS) It canbeseenthatthe least
restrictiveAS location isattheFourierplane(f 1
totherightof L1 f 2
to
lArrrArr
the
left
of
L2)
2
Given
the
following
GRIN
medium
2n(r) =
radic 2
minusr2
0lt r lt1
r=
radic x2 +z
1 r
ge1
(a) TheHamiltonianequationsare(r lt1)
dx =
partH 1 2P x
P x
P x
ds partP x
=
minus2
radic P x
2+P z
2
=
minusn
=
minusradic 2minusx2minusz2
dz =
partH
1 2P z
P z
P z
ds
partP z
=
minus2
radic P x
2+P z
2
=
minusn
=
minusradic 2minusx2minusz2
dP x
partH
1
minus2x x
x
= =
ds =
minus partx =
minus2
n n
radic 2minusx2minusz2
dP z
partH 1minus2z z z= =
ds
=
minuspartz
=
minus2 n n
radic 2minusx2minusz2
where
H =n(q )
minus[P 2 +P 2]12 = 0x z
=[2
minusx
2minus
z 2]12minus
[P x
2 +P z
2]12 = 0
n= P 2 +P 2
x z
2
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 39
(b) Recallthatwe justfoundn2 =P x
2 +P z
2 917501 2
917501 2
dP x
dP z
1048573x
11141092
1048573z 11141092 x2
+z 2 x2 +z 2
+ = + = =
ds ds n n n2 P 2 +P 2
x z
=
P
2
r
+
2
P
2 =
P
2
2minus
+
n
P
2
2 =
P
2 +
2
P
2minus
1
x z x z x z
partn
(c) Since =0theScreenHamiltonian isnotconserved Thismaybeverifiedby
partz
directsubstitution
h=
minus n2
minusP x
2 =
minus 2
minusx2
minusz 2minus
P x
2
andweseethatparth z
=
= 0
partz 2
minusx2
minusz 2
minusP x
2
3 ConsidertheMichelsoninterferometershownbelow
(a) Webeginbywritingtheanalyticexpression(inphasorform)of asphericalwave
withoriginat(x p z p)usingtheparaxialapproximation
E 0ei
2λπ
(zminuszp)
iπ
(xminusxp)2
E S = e
λ (zminuszp)
iλ(z minusz p)
For simplicity we take x p
= z p
= 0 At the observation plane the interference
patternisgivenby
I =
|E S 1
+E S 2
|2 =
|E S 1
|2 +
|E S 2
|2 +E S 1
E S lowast
2
+E S lowast
1
E S 2
3
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 49
917501
917501
917501
where
e λ π 2 e λ π
2E 0
i2π1
i x E 0
i
2π1
i xE S 1
= e
λ1 E S 2
= e
λ2
4 iλ1
4 iλ2
1
=z 0
+ 2z 1
+z c
2
=z 0
+ 2z 2
+z c
E 02 E 02
= =|E S 1
|2
16(λ1)2
|E S 2
|2
16(λ2)2
So
E 02 E 0
2 E 02
I = + + [e
i∆φ +eminusi∆φ]16(λ1)2
16(λ2)2 16λ212
E 02 1 1 2
=
16λ2 12
+
22
+
12
cos∆φ ∆φ=φ2
minusφ1
2π x2 2π x2
φ2 = +
2
φ1 = +
1λ
22
λ
21
2π 2
1 1rArr∆φ=
λ x
22
minus
21
+2∆z ∆z =z 2
minusz 1
917501
917501
E 02
1 1 2 2π 2
∆
I = + + cos xrArr
16λ2 21
22
12
λ 212
minus∆
∆=2∆z =2
minus1
E 02 1 1 2
I max
= + +
16λ2 21
22
12
E 02 1 1 2
I min
=
16λ2 2
1
+
22
minus
12
(b) If theflatmirrorM2isreplacedbyaconvexsphericalmirrorof radius2(z 0
+z 2)thesphericalwavegetscollimatedandtheinterferencepatternbecomes 2
E 0
E 0
2 E 0
2 E 0
2
I =E S 1
+ 4λ e
iφ
=
16(λ)2
+
16(λ1)2
+8λ21
sin∆φ
Plane
Wave Chirp
Function
4
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 59
=z 0
+z 2
2π
φ = 2λ
∆φ =φ1
minusφ
4
Consider
the
4-f
system
shown
below
(a) The pupil mask can be implemented by placing two pinholes (small apertures)onecenteredwithrespecttotheopticalaxisandthesecondoneat1cmoff-axisThe2ndpinholeisphasedelayedbyapieceof glassof thicknesstwhere
2πφ=π= t(15
minus1) t=λ
λ
rArr
(b) Theinputtransparencyis
=gt
middot 1048573 1048573 1048573 1048573 1048573 1048573 1114109
=1
α
infinsinc(αq )e
i2π
qx
gin
gillumination
Λ
q=minusinfin
AttheFourierplaneinfin 1048573
q 1114109Gin
=α sinc(αq )δ u
minus
Λ
u=
x
λf q=minusinfin 1048573 1114109 917501
917501
1
infin q λf λf 05
times10minus4
10
Gin(x) =
2
sinc
2
δ xminusq Λ
Λ
=
5
times10minus4
middot
= 1
q=minusinfin
5
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 69
917501
917501
917501
917501
917501
917501
Afterthepupilmaskonlythe0thand+1orderspass The+1ordergetsphase
delayed
byeiπ =
minus1
1 1 1
Gout(x) = δ (x)
minus sinc δ (xminus1)
2 2 2
1 1
δ (xminus
1)=
δ (x)
minus2 π
1 1
gout(u) =
2
minus
πeminusi2πu
u=
x
I out
=
1 1
2
minus
π
eminusi
2πx
λf
λf
2
1 1 1 2π x=
4
+
π2
minus
cos
π λ f
1 4π
Thecontrastisv= 0906=
π = 1 1+
4 +π2
4
π2
5
(a)
To
compute
the
OTF
we
first
need
the
ATF
u1
=
x=
1cm
= 02micromminus1 =200mmminus1
λf 05microm
times10cm
est
δx 02cm
δu=
λf asymp
05microm
times10cm
= 0025micromminus1 =25mmminus2
H (u) =H (u)
otimesH (u)
= rectu
minusrect
uminusu1
rect
uminusu
minusrect
uminusu1
minusu
du
δu
δu
δu
δu
(autocorrelation)
6
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 29
(c) Solution
Thenumericalapertureistanα
asympα
asympsinα
asympNA
asymp
a1
f 1
2X s
2f 1a2
2a2Thefieldof view(FOV)is FOV=2β = = =
3f 1
3f 1f 2
3f 2
(d)
The
location
of
S1
limits
the
FOV
because
of
the
requirement
for
the
CR
to
gothrough the center of the aperture stop (AS) It canbeseenthatthe least
restrictiveAS location isattheFourierplane(f 1
totherightof L1 f 2
to
lArrrArr
the
left
of
L2)
2
Given
the
following
GRIN
medium
2n(r) =
radic 2
minusr2
0lt r lt1
r=
radic x2 +z
1 r
ge1
(a) TheHamiltonianequationsare(r lt1)
dx =
partH 1 2P x
P x
P x
ds partP x
=
minus2
radic P x
2+P z
2
=
minusn
=
minusradic 2minusx2minusz2
dz =
partH
1 2P z
P z
P z
ds
partP z
=
minus2
radic P x
2+P z
2
=
minusn
=
minusradic 2minusx2minusz2
dP x
partH
1
minus2x x
x
= =
ds =
minus partx =
minus2
n n
radic 2minusx2minusz2
dP z
partH 1minus2z z z= =
ds
=
minuspartz
=
minus2 n n
radic 2minusx2minusz2
where
H =n(q )
minus[P 2 +P 2]12 = 0x z
=[2
minusx
2minus
z 2]12minus
[P x
2 +P z
2]12 = 0
n= P 2 +P 2
x z
2
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 39
(b) Recallthatwe justfoundn2 =P x
2 +P z
2 917501 2
917501 2
dP x
dP z
1048573x
11141092
1048573z 11141092 x2
+z 2 x2 +z 2
+ = + = =
ds ds n n n2 P 2 +P 2
x z
=
P
2
r
+
2
P
2 =
P
2
2minus
+
n
P
2
2 =
P
2 +
2
P
2minus
1
x z x z x z
partn
(c) Since =0theScreenHamiltonian isnotconserved Thismaybeverifiedby
partz
directsubstitution
h=
minus n2
minusP x
2 =
minus 2
minusx2
minusz 2minus
P x
2
andweseethatparth z
=
= 0
partz 2
minusx2
minusz 2
minusP x
2
3 ConsidertheMichelsoninterferometershownbelow
(a) Webeginbywritingtheanalyticexpression(inphasorform)of asphericalwave
withoriginat(x p z p)usingtheparaxialapproximation
E 0ei
2λπ
(zminuszp)
iπ
(xminusxp)2
E S = e
λ (zminuszp)
iλ(z minusz p)
For simplicity we take x p
= z p
= 0 At the observation plane the interference
patternisgivenby
I =
|E S 1
+E S 2
|2 =
|E S 1
|2 +
|E S 2
|2 +E S 1
E S lowast
2
+E S lowast
1
E S 2
3
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 49
917501
917501
917501
where
e λ π 2 e λ π
2E 0
i2π1
i x E 0
i
2π1
i xE S 1
= e
λ1 E S 2
= e
λ2
4 iλ1
4 iλ2
1
=z 0
+ 2z 1
+z c
2
=z 0
+ 2z 2
+z c
E 02 E 02
= =|E S 1
|2
16(λ1)2
|E S 2
|2
16(λ2)2
So
E 02 E 0
2 E 02
I = + + [e
i∆φ +eminusi∆φ]16(λ1)2
16(λ2)2 16λ212
E 02 1 1 2
=
16λ2 12
+
22
+
12
cos∆φ ∆φ=φ2
minusφ1
2π x2 2π x2
φ2 = +
2
φ1 = +
1λ
22
λ
21
2π 2
1 1rArr∆φ=
λ x
22
minus
21
+2∆z ∆z =z 2
minusz 1
917501
917501
E 02
1 1 2 2π 2
∆
I = + + cos xrArr
16λ2 21
22
12
λ 212
minus∆
∆=2∆z =2
minus1
E 02 1 1 2
I max
= + +
16λ2 21
22
12
E 02 1 1 2
I min
=
16λ2 2
1
+
22
minus
12
(b) If theflatmirrorM2isreplacedbyaconvexsphericalmirrorof radius2(z 0
+z 2)thesphericalwavegetscollimatedandtheinterferencepatternbecomes 2
E 0
E 0
2 E 0
2 E 0
2
I =E S 1
+ 4λ e
iφ
=
16(λ)2
+
16(λ1)2
+8λ21
sin∆φ
Plane
Wave Chirp
Function
4
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 59
=z 0
+z 2
2π
φ = 2λ
∆φ =φ1
minusφ
4
Consider
the
4-f
system
shown
below
(a) The pupil mask can be implemented by placing two pinholes (small apertures)onecenteredwithrespecttotheopticalaxisandthesecondoneat1cmoff-axisThe2ndpinholeisphasedelayedbyapieceof glassof thicknesstwhere
2πφ=π= t(15
minus1) t=λ
λ
rArr
(b) Theinputtransparencyis
=gt
middot 1048573 1048573 1048573 1048573 1048573 1048573 1114109
=1
α
infinsinc(αq )e
i2π
qx
gin
gillumination
Λ
q=minusinfin
AttheFourierplaneinfin 1048573
q 1114109Gin
=α sinc(αq )δ u
minus
Λ
u=
x
λf q=minusinfin 1048573 1114109 917501
917501
1
infin q λf λf 05
times10minus4
10
Gin(x) =
2
sinc
2
δ xminusq Λ
Λ
=
5
times10minus4
middot
= 1
q=minusinfin
5
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 69
917501
917501
917501
917501
917501
917501
Afterthepupilmaskonlythe0thand+1orderspass The+1ordergetsphase
delayed
byeiπ =
minus1
1 1 1
Gout(x) = δ (x)
minus sinc δ (xminus1)
2 2 2
1 1
δ (xminus
1)=
δ (x)
minus2 π
1 1
gout(u) =
2
minus
πeminusi2πu
u=
x
I out
=
1 1
2
minus
π
eminusi
2πx
λf
λf
2
1 1 1 2π x=
4
+
π2
minus
cos
π λ f
1 4π
Thecontrastisv= 0906=
π = 1 1+
4 +π2
4
π2
5
(a)
To
compute
the
OTF
we
first
need
the
ATF
u1
=
x=
1cm
= 02micromminus1 =200mmminus1
λf 05microm
times10cm
est
δx 02cm
δu=
λf asymp
05microm
times10cm
= 0025micromminus1 =25mmminus2
H (u) =H (u)
otimesH (u)
= rectu
minusrect
uminusu1
rect
uminusu
minusrect
uminusu1
minusu
du
δu
δu
δu
δu
(autocorrelation)
6
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 39
(b) Recallthatwe justfoundn2 =P x
2 +P z
2 917501 2
917501 2
dP x
dP z
1048573x
11141092
1048573z 11141092 x2
+z 2 x2 +z 2
+ = + = =
ds ds n n n2 P 2 +P 2
x z
=
P
2
r
+
2
P
2 =
P
2
2minus
+
n
P
2
2 =
P
2 +
2
P
2minus
1
x z x z x z
partn
(c) Since =0theScreenHamiltonian isnotconserved Thismaybeverifiedby
partz
directsubstitution
h=
minus n2
minusP x
2 =
minus 2
minusx2
minusz 2minus
P x
2
andweseethatparth z
=
= 0
partz 2
minusx2
minusz 2
minusP x
2
3 ConsidertheMichelsoninterferometershownbelow
(a) Webeginbywritingtheanalyticexpression(inphasorform)of asphericalwave
withoriginat(x p z p)usingtheparaxialapproximation
E 0ei
2λπ
(zminuszp)
iπ
(xminusxp)2
E S = e
λ (zminuszp)
iλ(z minusz p)
For simplicity we take x p
= z p
= 0 At the observation plane the interference
patternisgivenby
I =
|E S 1
+E S 2
|2 =
|E S 1
|2 +
|E S 2
|2 +E S 1
E S lowast
2
+E S lowast
1
E S 2
3
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 49
917501
917501
917501
where
e λ π 2 e λ π
2E 0
i2π1
i x E 0
i
2π1
i xE S 1
= e
λ1 E S 2
= e
λ2
4 iλ1
4 iλ2
1
=z 0
+ 2z 1
+z c
2
=z 0
+ 2z 2
+z c
E 02 E 02
= =|E S 1
|2
16(λ1)2
|E S 2
|2
16(λ2)2
So
E 02 E 0
2 E 02
I = + + [e
i∆φ +eminusi∆φ]16(λ1)2
16(λ2)2 16λ212
E 02 1 1 2
=
16λ2 12
+
22
+
12
cos∆φ ∆φ=φ2
minusφ1
2π x2 2π x2
φ2 = +
2
φ1 = +
1λ
22
λ
21
2π 2
1 1rArr∆φ=
λ x
22
minus
21
+2∆z ∆z =z 2
minusz 1
917501
917501
E 02
1 1 2 2π 2
∆
I = + + cos xrArr
16λ2 21
22
12
λ 212
minus∆
∆=2∆z =2
minus1
E 02 1 1 2
I max
= + +
16λ2 21
22
12
E 02 1 1 2
I min
=
16λ2 2
1
+
22
minus
12
(b) If theflatmirrorM2isreplacedbyaconvexsphericalmirrorof radius2(z 0
+z 2)thesphericalwavegetscollimatedandtheinterferencepatternbecomes 2
E 0
E 0
2 E 0
2 E 0
2
I =E S 1
+ 4λ e
iφ
=
16(λ)2
+
16(λ1)2
+8λ21
sin∆φ
Plane
Wave Chirp
Function
4
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 59
=z 0
+z 2
2π
φ = 2λ
∆φ =φ1
minusφ
4
Consider
the
4-f
system
shown
below
(a) The pupil mask can be implemented by placing two pinholes (small apertures)onecenteredwithrespecttotheopticalaxisandthesecondoneat1cmoff-axisThe2ndpinholeisphasedelayedbyapieceof glassof thicknesstwhere
2πφ=π= t(15
minus1) t=λ
λ
rArr
(b) Theinputtransparencyis
=gt
middot 1048573 1048573 1048573 1048573 1048573 1048573 1114109
=1
α
infinsinc(αq )e
i2π
qx
gin
gillumination
Λ
q=minusinfin
AttheFourierplaneinfin 1048573
q 1114109Gin
=α sinc(αq )δ u
minus
Λ
u=
x
λf q=minusinfin 1048573 1114109 917501
917501
1
infin q λf λf 05
times10minus4
10
Gin(x) =
2
sinc
2
δ xminusq Λ
Λ
=
5
times10minus4
middot
= 1
q=minusinfin
5
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 69
917501
917501
917501
917501
917501
917501
Afterthepupilmaskonlythe0thand+1orderspass The+1ordergetsphase
delayed
byeiπ =
minus1
1 1 1
Gout(x) = δ (x)
minus sinc δ (xminus1)
2 2 2
1 1
δ (xminus
1)=
δ (x)
minus2 π
1 1
gout(u) =
2
minus
πeminusi2πu
u=
x
I out
=
1 1
2
minus
π
eminusi
2πx
λf
λf
2
1 1 1 2π x=
4
+
π2
minus
cos
π λ f
1 4π
Thecontrastisv= 0906=
π = 1 1+
4 +π2
4
π2
5
(a)
To
compute
the
OTF
we
first
need
the
ATF
u1
=
x=
1cm
= 02micromminus1 =200mmminus1
λf 05microm
times10cm
est
δx 02cm
δu=
λf asymp
05microm
times10cm
= 0025micromminus1 =25mmminus2
H (u) =H (u)
otimesH (u)
= rectu
minusrect
uminusu1
rect
uminusu
minusrect
uminusu1
minusu
du
δu
δu
δu
δu
(autocorrelation)
6
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 49
917501
917501
917501
where
e λ π 2 e λ π
2E 0
i2π1
i x E 0
i
2π1
i xE S 1
= e
λ1 E S 2
= e
λ2
4 iλ1
4 iλ2
1
=z 0
+ 2z 1
+z c
2
=z 0
+ 2z 2
+z c
E 02 E 02
= =|E S 1
|2
16(λ1)2
|E S 2
|2
16(λ2)2
So
E 02 E 0
2 E 02
I = + + [e
i∆φ +eminusi∆φ]16(λ1)2
16(λ2)2 16λ212
E 02 1 1 2
=
16λ2 12
+
22
+
12
cos∆φ ∆φ=φ2
minusφ1
2π x2 2π x2
φ2 = +
2
φ1 = +
1λ
22
λ
21
2π 2
1 1rArr∆φ=
λ x
22
minus
21
+2∆z ∆z =z 2
minusz 1
917501
917501
E 02
1 1 2 2π 2
∆
I = + + cos xrArr
16λ2 21
22
12
λ 212
minus∆
∆=2∆z =2
minus1
E 02 1 1 2
I max
= + +
16λ2 21
22
12
E 02 1 1 2
I min
=
16λ2 2
1
+
22
minus
12
(b) If theflatmirrorM2isreplacedbyaconvexsphericalmirrorof radius2(z 0
+z 2)thesphericalwavegetscollimatedandtheinterferencepatternbecomes 2
E 0
E 0
2 E 0
2 E 0
2
I =E S 1
+ 4λ e
iφ
=
16(λ)2
+
16(λ1)2
+8λ21
sin∆φ
Plane
Wave Chirp
Function
4
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 59
=z 0
+z 2
2π
φ = 2λ
∆φ =φ1
minusφ
4
Consider
the
4-f
system
shown
below
(a) The pupil mask can be implemented by placing two pinholes (small apertures)onecenteredwithrespecttotheopticalaxisandthesecondoneat1cmoff-axisThe2ndpinholeisphasedelayedbyapieceof glassof thicknesstwhere
2πφ=π= t(15
minus1) t=λ
λ
rArr
(b) Theinputtransparencyis
=gt
middot 1048573 1048573 1048573 1048573 1048573 1048573 1114109
=1
α
infinsinc(αq )e
i2π
qx
gin
gillumination
Λ
q=minusinfin
AttheFourierplaneinfin 1048573
q 1114109Gin
=α sinc(αq )δ u
minus
Λ
u=
x
λf q=minusinfin 1048573 1114109 917501
917501
1
infin q λf λf 05
times10minus4
10
Gin(x) =
2
sinc
2
δ xminusq Λ
Λ
=
5
times10minus4
middot
= 1
q=minusinfin
5
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 69
917501
917501
917501
917501
917501
917501
Afterthepupilmaskonlythe0thand+1orderspass The+1ordergetsphase
delayed
byeiπ =
minus1
1 1 1
Gout(x) = δ (x)
minus sinc δ (xminus1)
2 2 2
1 1
δ (xminus
1)=
δ (x)
minus2 π
1 1
gout(u) =
2
minus
πeminusi2πu
u=
x
I out
=
1 1
2
minus
π
eminusi
2πx
λf
λf
2
1 1 1 2π x=
4
+
π2
minus
cos
π λ f
1 4π
Thecontrastisv= 0906=
π = 1 1+
4 +π2
4
π2
5
(a)
To
compute
the
OTF
we
first
need
the
ATF
u1
=
x=
1cm
= 02micromminus1 =200mmminus1
λf 05microm
times10cm
est
δx 02cm
δu=
λf asymp
05microm
times10cm
= 0025micromminus1 =25mmminus2
H (u) =H (u)
otimesH (u)
= rectu
minusrect
uminusu1
rect
uminusu
minusrect
uminusu1
minusu
du
δu
δu
δu
δu
(autocorrelation)
6
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 59
=z 0
+z 2
2π
φ = 2λ
∆φ =φ1
minusφ
4
Consider
the
4-f
system
shown
below
(a) The pupil mask can be implemented by placing two pinholes (small apertures)onecenteredwithrespecttotheopticalaxisandthesecondoneat1cmoff-axisThe2ndpinholeisphasedelayedbyapieceof glassof thicknesstwhere
2πφ=π= t(15
minus1) t=λ
λ
rArr
(b) Theinputtransparencyis
=gt
middot 1048573 1048573 1048573 1048573 1048573 1048573 1114109
=1
α
infinsinc(αq )e
i2π
qx
gin
gillumination
Λ
q=minusinfin
AttheFourierplaneinfin 1048573
q 1114109Gin
=α sinc(αq )δ u
minus
Λ
u=
x
λf q=minusinfin 1048573 1114109 917501
917501
1
infin q λf λf 05
times10minus4
10
Gin(x) =
2
sinc
2
δ xminusq Λ
Λ
=
5
times10minus4
middot
= 1
q=minusinfin
5
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 69
917501
917501
917501
917501
917501
917501
Afterthepupilmaskonlythe0thand+1orderspass The+1ordergetsphase
delayed
byeiπ =
minus1
1 1 1
Gout(x) = δ (x)
minus sinc δ (xminus1)
2 2 2
1 1
δ (xminus
1)=
δ (x)
minus2 π
1 1
gout(u) =
2
minus
πeminusi2πu
u=
x
I out
=
1 1
2
minus
π
eminusi
2πx
λf
λf
2
1 1 1 2π x=
4
+
π2
minus
cos
π λ f
1 4π
Thecontrastisv= 0906=
π = 1 1+
4 +π2
4
π2
5
(a)
To
compute
the
OTF
we
first
need
the
ATF
u1
=
x=
1cm
= 02micromminus1 =200mmminus1
λf 05microm
times10cm
est
δx 02cm
δu=
λf asymp
05microm
times10cm
= 0025micromminus1 =25mmminus2
H (u) =H (u)
otimesH (u)
= rectu
minusrect
uminusu1
rect
uminusu
minusrect
uminusu1
minusu
du
δu
δu
δu
δu
(autocorrelation)
6
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 69
917501
917501
917501
917501
917501
917501
Afterthepupilmaskonlythe0thand+1orderspass The+1ordergetsphase
delayed
byeiπ =
minus1
1 1 1
Gout(x) = δ (x)
minus sinc δ (xminus1)
2 2 2
1 1
δ (xminus
1)=
δ (x)
minus2 π
1 1
gout(u) =
2
minus
πeminusi2πu
u=
x
I out
=
1 1
2
minus
π
eminusi
2πx
λf
λf
2
1 1 1 2π x=
4
+
π2
minus
cos
π λ f
1 4π
Thecontrastisv= 0906=
π = 1 1+
4 +π2
4
π2
5
(a)
To
compute
the
OTF
we
first
need
the
ATF
u1
=
x=
1cm
= 02micromminus1 =200mmminus1
λf 05microm
times10cm
est
δx 02cm
δu=
λf asymp
05microm
times10cm
= 0025micromminus1 =25mmminus2
H (u) =H (u)
otimesH (u)
= rectu
minusrect
uminusu1
rect
uminusu
minusrect
uminusu1
minusu
du
δu
δu
δu
δu
(autocorrelation)
6
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 79
917501
917501
917501 917501
=
rect
urect
uminusu
duδu δu
rarr
917501 917501
rect
u minusrect
uminusu1
minusu
duminus
δu δu
rarr
917501
917501
rect
uminusu1
rectuminusu
duminus
δu δu
rarr
917501 917501
+ rect
uminusu1
rect
uminusu1
minusu
duδu δu
rarr
SotheresultantOTFandMTFare(afternormalization)
(b) OnlytheDCandthe
plusmn1stharmonicsatu=
plusmn200mmminus1 (period=5microm)ie
1 1 1 2πx I (x) =
2
minus
2
times
π
times2cos
5microm
=
DC
term
minusH (200mmminus2)
times
1st
harmonic
times
2
cos
2πx
5microm
(c) Solution
7
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 89
F minusrarr sinc2(δux)sotheiPSFis
1048573 1114109
1048573 1114109
x x =sinc2
40microm
times 1
minuscos 2π
5microm
8
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms
8102019 MIT2 71S09 Gfinal Sol
httpslidepdfcomreaderfullmit2-71s09-gfinal-sol 99
MIT OpenCourseWarehttpocwmitedu
271 2710 OpticsSpring 2009
For information about citing these materials or our Terms of Use visit httpocwmiteduterms