![Page 1: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/1.jpg)
Today’s Outline - November 21, 2016
• Imaging
• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 2: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/2.jpg)
Today’s Outline - November 21, 2016
• Imaging
• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 3: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/3.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography
• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 4: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/4.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy
• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 5: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/5.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging
• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 6: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/6.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry
• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 7: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/7.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging
• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 8: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/8.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 9: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/9.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 10: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/10.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 11: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/11.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the exam
Send me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 12: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/12.jpg)
Today’s Outline - November 21, 2016
• Imaging• Computed tomography• Microscopy• Phase contrast imaging• Grating interferometry• Coherent diffraction imaging• Holography
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change)
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 1 / 24
![Page 13: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/13.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 14: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/14.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 15: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/15.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 16: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/16.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 17: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/17.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 18: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/18.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 19: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/19.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 20: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/20.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 21: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/21.jpg)
Phase difference in scattering
R
a
P
F
O
D
F
ψk
k
r
All imaging can be broken into athree step process
1 x-ray interaction with sample
2 scattered x-ray propagation
3 interaction with detector
The scattered waves from O and Pwill travel different distances
In the far field, the phase differenceis φ ≈ ~Q ·~r with ~Q = ~k ′ − ~k
Since ~k ⊥ ~r , φ ≈ ~Q ·~r = ~k ′ ·~r
The path length difference corresponding to this phase shift is k ′ · r = OF ′
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24
![Page 22: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/22.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
![Page 23: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/23.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
![Page 24: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/24.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
![Page 25: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/25.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2
=a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
![Page 26: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/26.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
![Page 27: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/27.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
![Page 28: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/28.jpg)
Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
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Franuhofer, Fresnel, and contact regimes
R
a
P
F
O
D
F
ψk
k
r
The path length difference computed with the far field approximation hasa built in error of ∆ = FF ′ which sets a scale for different kinds of imaging
∆ = R − R cosψ
≈ R(1− (1− ψ2/2))
= Ra2
2R2=
a2
2R
R � a2
λFraunhofer
R ≈ a2
λFresnel
R � a2
λContact
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 3 / 24
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Detector placement
R
a
P
F
O
D
F
ψk
k
r
If λ = 1 A and the distance to be resolved is a = 1 A, then a2/λ = 1 Aand any detector placement is in the Fraunhofer (far field) regime
if a = µm, then a2/λ = 10 mm and the imaging regime can be selected bydetector placement
if a = 1 mm, then a2/λ = 10 km and the detector will always be in thecontact regime
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 4 / 24
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Detector placement
R
a
P
F
O
D
F
ψk
k
r
If λ = 1 A and the distance to be resolved is a = 1 A, then a2/λ = 1 Aand any detector placement is in the Fraunhofer (far field) regime
if a = µm, then a2/λ = 10 mm and the imaging regime can be selected bydetector placement
if a = 1 mm, then a2/λ = 10 km and the detector will always be in thecontact regime
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 4 / 24
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Detector placement
R
a
P
F
O
D
F
ψk
k
r
If λ = 1 A and the distance to be resolved is a = 1 A, then a2/λ = 1 Aand any detector placement is in the Fraunhofer (far field) regime
if a = µm, then a2/λ = 10 mm and the imaging regime can be selected bydetector placement
if a = 1 mm, then a2/λ = 10 km and the detector will always be in thecontact regime
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 4 / 24
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Contact to far-field imaging
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 5 / 24
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Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895.
In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
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Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895. In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
![Page 36: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/36.jpg)
Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895. In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)
The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
![Page 37: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/37.jpg)
Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895. In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
![Page 38: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/38.jpg)
Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895. In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
![Page 39: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/39.jpg)
Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895. In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
![Page 40: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/40.jpg)
Radiography to tomography
Radiography started immedi-ately after the discovery ofx-rays in 1895. In 1970Computer Tomography revo-lutionized x-ray imaging
Assume the object to be im-aged has a non uniform ab-sorption coefficient µ(x , y)The line integral of the ab-sorption coefficient at a par-ticular value of x ′ is mea-sured as the ratio of thetransmitted to the incidentbeam
I = I0e−
∫µ(x ,y)dy ′
ln
(I0I
)=
∫µ(x , y)dy ′
The radon transform R(θ, x ′) is used to reconstruct the 3D absorptionimage of the object numerically.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 6 / 24
![Page 41: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/41.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
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Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
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Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 44: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/44.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 45: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/45.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)?
The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 46: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/46.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy )
and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 47: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/47.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy )
and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 48: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/48.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 49: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/49.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx
=
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 50: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/50.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx
= P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 51: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/51.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
![Page 52: Today’s Outline - November 21, 2016phys.iit.edu/~segre/phys570/16F/lecture_24.pdfC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 2 / 24. Phase di erence in scattering R a P](https://reader035.vdocuments.us/reader035/viewer/2022070212/6105019af11e20487b69d3b1/html5/thumbnails/52.jpg)
Fourier slice theorem
Start with a general functionf (x , y) which is projected onto thex-axis
the Fourier transform of the projec-tion is
p(x) =
∫f (x , y)dy
P(qx) =
∫p(x)e iqxxdx
What is the relationship of the Fourier transform, P(qx), to the originalfunction, f (x , y)? The Fourier transform of f (x , y) is F (qx , qy ) and bychoosing qy ≡ 0, we get a slice
F (qx , qy ) =
∫ ∫f (x , y)e iqxx+qyydxdy
F (qx , qy = 0) =
∫ [∫f (x , y)dy
]e iqxxdx =
∫p(x)e iqxxdx = P(qx)
The Fourier transform of the projection is equal to a slice through theFourier transform of the object at the origin in the direction of propagation
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 7 / 24
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Fourier transform reconstruction
Fourier transform
Slice
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 8 / 24
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Sinograms
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 9 / 24
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Medical tomography
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 10 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM
= 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf
= 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D
= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Microscopy
The radius of the mth zone isrm ≈
√mλf
the width of the outermostzone is
∆rM =√λf (√M −
√M − 1)
≈√λf
2√M
f = 4M(∆rM)2
λ
D = 2rM = 2√Mλf
= 2√M√λf = 4M∆rM
∆x = 1.22λf
D= 1.22∆rM
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 11 / 24
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Scanning transmission x-ray microscope
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 12 / 24
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Full field microscope
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 13 / 24
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Transmission x-ray microscope
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 14 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n
=λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ
≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x
≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from refraction
When x-rays cross an inter-face that is not normal totheir direction, there is re-fraction
The angle of refraction α canbe calculated
λn =λ
n=
λ
1− δ≈ λ(1 + δ)
α =λ(1 + δ)− λ
∆x
= δλ
∆x≈ δ tanω
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 15 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂xcompare to αrefrac = λ
δ
∆x
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂xcompare to αrefrac = λ
δ
∆x
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x
=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂xcompare to αrefrac = λ
δ
∆x
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x
=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂xcompare to αrefrac = λ
δ
∆x
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂xcompare to αrefrac = λ
δ
∆x
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂x
compare to αrefrac = λδ
∆x
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Angular deviation from graded density
In a similar way, there isan angular deviation whenthe material density variesnormal to the propagationdirection
The angle of refraction αcan be calculated
α =λ(1 + δ(x + ∆x))− λ(1 + δ(x))
∆x=λ∆x ∂δ(x)∂x
∆x
δ(x + ∆x) ≈ δ(x) + ∆x∂δ(x)
∂x
αgradient = λ∂δ(x)
∂xcompare to αrefrac = λ
δ
∆xC. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 16 / 24
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′=
λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′
=λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 17 / 24
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′=
λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 17 / 24
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′=
λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 17 / 24
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′=
λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 17 / 24
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′=
λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 17 / 24
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Phase shift from angular deviation
This deviation of the x-ray beam, leads to a phase shift φ(~r) = ~k ′ ·~r at aspecific position along the original propagation direction z
n =~k ′
k ′=
λ
2π∇φ(~r)
αx =λ
2π
∂φ(x , y)
∂x
αy =λ
2π
∂φ(x , y)
∂y
Thus the angular deviation, in eachof the x and y directions in theplane perpendicular to the originalpropagation direction becomes
By measuring the angular deviationas a function of position in a sam-ple, one can reconstruct the phaseshift φ(x , y) due to the sample byintegration.
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 17 / 24
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Phase contrast experiment
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Phase contrast experiment
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Imaging a silicon trough
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Imaging blood cells
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 22 / 24
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 22 / 24
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Wavefield propagation
In order to understand many of these imaging techniques, it is importantto have a good model for wave propagation in an optical system
start with a monochromatic plane wave propagating in the z direction,described by the function e ikz with wavelength λ = 2π/k
when the wavefront passes through an optical element or a sample, it isdistorted such that the wavefield at z = 0 is now a function of thetransverse dimensions, x and y : ψ0(x , y)
our goal is to determine the wavefield at a distance z downstream and thisis done by constructing a propagation operator Dz such that
ψz = Dzψ0(x , y)
The Fourier transform is used to generate this propagation operator in thefollowing way (showing only the x dependence for simplicity)
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 22 / 24
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√
k2 − k2x ≈ k − k2x2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√
k2 − k2x ≈ k − k2x2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows
but if kx � k we have
kz =√
k2 − k2x ≈ k − k2x2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows
but if kx � k we have
kz =√k2 − k2x
≈ k − k2x2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x
≈ k − k2x2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 23 / 24
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz
= ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 23 / 24
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 23 / 24
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)]
=1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 23 / 24
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
C. Segre (IIT) PHYS 570 - Fall 2016 November 21, 2016 23 / 24
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Wavefield propagation
ψ0(x) =1
2π
∫ψ0(kx)e−ikxxdkx
in words, this says that at z = 0 the wavefield is a superposition of planewaves each of which is a function of the total wavevector ~k = kx x + kz z
We can rewrite the relationships as follows but if kx � k we have
kz =√k2 − k2x ≈ k − k2x
2k
each of the plane waves ψ0e−ikxx propagates to z by multiplication with a
phase factor
ψ0e−ikxx → ψ0e
−ikxxe ikzz = ψ0e−ikxxe ikze−ik
2x z/2k = ψz(kx)
ψz(x) = FT −1[ψz(kx)] =1
2π
∫ψz(kx)e−ikxxdkx
ψz(x , y) = Dzψ0(x , y) = e ikz FT −1[e−iz(k
2x+k2
y )/2k FT [ψ0(x , y)]]
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Fresnel zone plates
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Fresnel zone plates
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