PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia...
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Transcript of PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia...
![Page 1: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/1.jpg)
PC20312 Wave Optics
Section 4:
Diffraction
![Page 2: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/2.jpg)
Huygens-Fresnel Principle I
Image from Wikipedia
Augustin-Jean Fresnel 1788-1827
“Every unobstructed point of a wavefront… serves as a source of spherical secondary wavelets … The amplitude of the optical field at any point beyond is the superposition of all these wavelets ...”
• Fresnel combined ideas of Huygens’ wavelets & interference
• Postulated in 1818:
Hecht, p444
![Page 3: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/3.jpg)
Huygens-Fresnel Principle II
Gustav R. Kirchhoff
1824-1887
• Fresnel’s postulate (1818) predates Maxwell’s equations (1861)
• Formally derived from the scalar wave equation by Kirchoff in 1882
• Worked with Schuster for year at the University of Heidelberg
Image from Wikipedia
![Page 4: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/4.jpg)
Huygens-Fresnel Principle III
Total area, A
P
dA1
dA3dA2
Optical field at P depends on the superposition of contributions from each elemental area dA of
the total area A
![Page 5: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/5.jpg)
Huygens-Fresnel Principle IV
Divide an aperture into elemental areas each of which is a source of a spherical wavelet
Image from Wikipedia
http://www.acoustics.salford.ac.uk/feschools/waves/diffract3.htm
![Page 6: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/6.jpg)
The Huygens-Fresnel Integral
Source, S Observation point, P
Q
Spherical wavefront
s r
s0 R
![Page 7: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/7.jpg)
Fraunhofer diffraction
Joseph von Fraunhofer
1787-1826
The case of small, linear phase variation, i.e.:
• r R + r ,
• r << R
• r x,y
Satisfied when s,r >> d
Hence, “Far-field diffraction”
Image from Wikipedia
y
x
aperture
d
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Far-field diffraction
S
s0
• s0 >> d
• wavefront plane at aperture
• s s0
P
d D
• R >>d
• const. set K() 1
• D >> d
R
![Page 9: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/9.jpg)
Analysis of Fraunhofer diffraction
Source, S
Observation point, P(X,Y)
Q(x,y)
s
r
R
s0 Z
Aperture, A(x,y)
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Single slit diffractiony
xa/2-a/2
Image from Wikipedia
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Rectangular aperturey
xa/2-a/2
b/2
-b/2
Image from Wikipedia
![Page 12: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/12.jpg)
Circular aperture Iy
xa
u
Image from Wikipedia
Airy disc
Airy rings
The Airy Pattern
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Circular aperture II
-10 -5 0 5 100
0.2
0.4
0.6
0.8
1
No
rma
lise
d I
nte
nsi
ty
ka
kaθD=3.83I=0.0175I(0)
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The diffraction limit
f
f Image from Google Images
If there was no diffraction:
• parallel rays focused to a point
• images would be perfectly sharp
BUT, diffraction from instrumental apertures :
• produce rays at a range of angles
• which are focused at different points
• image is thus smeared out.
Even for a perfect optical system, diffraction limits
resolution.
![Page 15: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/15.jpg)
Radius of the Airy disc
f
D
Radius, RA= fD = 1.22f/d
Fraunhofer diffraction patterns also formed in focal plane of a lens¶
¶ e.g. see ‘Modern Optics’ by R Guenther
Appendix 10-A
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Two finite slits
E2(X)
E1(X)
E1(X)E2(X)
d
R
x
X
aa
Image courtesy of A Pedlar
![Page 17: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/17.jpg)
Point spread function
Images courtesy of A Pedlar & from Wikipedia
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The diffraction grating
David Rittenhouse 1732-1796
• Rittenhouse 1785:
• fine threads between screws – 100 threads/inch
• Fraunhofer 1821:
• thin wires
• Henry Augustus Rowland:
• curved gratings
• spectrocopy
• Henry Joseph Grayson 1899:
• developed precise ‘ruling engine’
• 120,000 lines/inch
Henry Augustus Rowland 1848-1901
A periodic structure designed to diffract light
Images from Wikipedia
![Page 19: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/19.jpg)
Grating structure
Ruled grating
Blazed grating – enhances diffraction in one direction
Gratings:
• central to modern spectrometers
• reflection or transmission
• amplitude or phase
Phase grating
0 5 10 15Distance
Ref
ract
ive
inde
x
![Page 20: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/20.jpg)
Analysis of diffraction from gratings
d
d
1 2
Path length difference for incident rays: Path length difference for diffracted rays:
d
1
2
![Page 21: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/21.jpg)
Modern gratings
Reflection gratings
Transmission gratings
CDs / DVDsImages from Wikipedia
![Page 22: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/22.jpg)
Gratings in nature
Nacre
Peacock feathers
Butterfly wings
Images from Wikipedia
![Page 23: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/23.jpg)
Grating based spectrometers
The Czerny-Turner monochromator.
• A – input light
• B – entrance slit
• C – collimating mirror
• D – diffraction grating
• E – focusing mirror
• F – exit slit
• G – output light
Image from Wikipedia
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General diffraction (again)
Source, S Observation point, P
Q
Spherical wavefront
s r
s0 R
![Page 25: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/25.jpg)
Half-period zones
s
S
P
rm+1
rm
rm
rm+1
S P
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Area of the mth zone
S
ds
sd
ssin
P
ssin
ssind
S
s
P
rm
s+R
![Page 27: PC20312 Wave Optics Section 4: Diffraction. Huygens-Fresnel Principle I Image from Wikipedia Augustin-Jean Fresnel 1788-1827 “Every unobstructed point.](https://reader030.fdocuments.in/reader030/viewer/2022032517/56649c9d5503460f9495c222/html5/thumbnails/27.jpg)
Zone plates
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Arago’s spot
François Jean Dominique Arago (1783-1856)
Siméon Denis Poisson (1781 -1840)
http://demo.physics.uiuc.edu/LectDemo/scripts/demo_descript.idc?DemoID=749
Merde !
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Fresnel diffraction from straight edges
y
x
Q(x,y)
S
s
P
r
Q(x,y)
s0 R