longitudinal coherence - synchrotron radiation...
TRANSCRIPT
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ
2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ
−→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ
−→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ
−→ LL =λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Longitudinal Coherence
Definition: Distance over which two waves from the same source pointwith slightly different wavelengths will completely dephase.
λ
λ−∆λ
P
2LL
Two waves of slightly different wavelengthsλ and λ−∆λ are emitted from the samepoint in space simultaneously.
After a distance LL, the two waves will beexactly out of phase and after 2LL they willonce again be in phase.
2LL = Nλ2LL = (N + 1)(λ−∆λ)
Nλ = Nλ+ λ− N∆λ−∆λ
0 = λ−N∆λ−∆λ −→ λ = (N + 1)∆λ −→ N ≈ λ
∆λ−→ LL =
λ2
2∆λ
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 1 / 8
Transverse Coherence
Definition: The lateral distance along a wavefront over which there is acomplete dephasing between two waves, of the same wavelngth, whichoriginate from two separate points in space.
λ
D
∆θ
2LT
P
R
∆θ
If we assume that the two wavesoriginate from points with a smallangular separation ∆θ, Thetransverse coherence length is givenby:
λ
2LT= tan ∆θ ≈ ∆θ
D
R= tan ∆θ ≈ ∆θ
LT =λR
2D
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 2 / 8
Transverse Coherence
Definition: The lateral distance along a wavefront over which there is acomplete dephasing between two waves, of the same wavelngth, whichoriginate from two separate points in space.
λ
D
∆θ
2LT
P
R
∆θ
If we assume that the two wavesoriginate from points with a smallangular separation ∆θ, Thetransverse coherence length is givenby:
λ
2LT= tan ∆θ ≈ ∆θ
D
R= tan ∆θ ≈ ∆θ
LT =λR
2D
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 2 / 8
Transverse Coherence
Definition: The lateral distance along a wavefront over which there is acomplete dephasing between two waves, of the same wavelngth, whichoriginate from two separate points in space.
λ
D
∆θ
2LT
P
R
∆θ
If we assume that the two wavesoriginate from points with a smallangular separation ∆θ, Thetransverse coherence length is givenby:
λ
2LT= tan ∆θ
≈ ∆θ
D
R= tan ∆θ
≈ ∆θ
LT =λR
2D
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 2 / 8
Transverse Coherence
Definition: The lateral distance along a wavefront over which there is acomplete dephasing between two waves, of the same wavelngth, whichoriginate from two separate points in space.
λ
D
∆θ
2LT
P
R
∆θ
If we assume that the two wavesoriginate from points with a smallangular separation ∆θ, Thetransverse coherence length is givenby:
λ
2LT= tan ∆θ ≈ ∆θ
D
R= tan ∆θ ≈ ∆θ
LT =λR
2D
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 2 / 8
Transverse Coherence
Definition: The lateral distance along a wavefront over which there is acomplete dephasing between two waves, of the same wavelngth, whichoriginate from two separate points in space.
λ
D
∆θ
2LT
P
R
∆θ
If we assume that the two wavesoriginate from points with a smallangular separation ∆θ, Thetransverse coherence length is givenby:
λ
2LT= tan ∆θ ≈ ∆θ
D
R= tan ∆θ ≈ ∆θ
LT =λR
2D
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 2 / 8
Coherence Lengths at the APS
For a typical 3rd generation undulator source, such as at the AdvancedPhoton Source the vertical source size is D = 100µm and we are typicallyR = 50m away with our experiment. If we assume a typical wavelength ofλ = 1A, and a monochromator resolution of ∆λ/λ = 10−5 we have for thevertical direction:
LL =1× 10−10
2 · 10−5= 5µm
LT =(1× 10−10) · 50
2 · (100× 10−6)= 25µm
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 3 / 8
Coherence Lengths at the APS
For a typical 3rd generation undulator source, such as at the AdvancedPhoton Source the vertical source size is D = 100µm and we are typicallyR = 50m away with our experiment. If we assume a typical wavelength ofλ = 1A, and a monochromator resolution of ∆λ/λ = 10−5 we have for thevertical direction:
LL =1× 10−10
2 · 10−5= 5µm
LT =(1× 10−10) · 50
2 · (100× 10−6)= 25µm
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 3 / 8
Coherence Lengths at the APS
For a typical 3rd generation undulator source, such as at the AdvancedPhoton Source the vertical source size is D = 100µm and we are typicallyR = 50m away with our experiment. If we assume a typical wavelength ofλ = 1A, and a monochromator resolution of ∆λ/λ = 10−5 we have for thevertical direction:
LL =1× 10−10
2 · 10−5= 5µm
LT =(1× 10−10) · 50
2 · (100× 10−6)= 25µm
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 3 / 8
X-Ray Tube Schematics
Fixed anode tube
Rotating anode tube
• low power
• low maintenance
• high power
• high maintenance
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 4 / 8
X-Ray Tube Schematics
Fixed anode tube Rotating anode tube
• low power
• low maintenance
• high power
• high maintenance
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 4 / 8
X-Ray Tube Spectrum
• Characteristic energy ofelemental fluorescenceemission
• Minimum wavelength(maximum energy) set byaccelerating potential
• Bremsstrahlung radiationprovides smoothbackground
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 5 / 8
X-Ray Tube Spectrum
• Characteristic energy ofelemental fluorescenceemission
• Minimum wavelength(maximum energy) set byaccelerating potential
• Bremsstrahlung radiationprovides smoothbackground
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 5 / 8
X-Ray Tube Spectrum
• Characteristic energy ofelemental fluorescenceemission
• Minimum wavelength(maximum energy) set byaccelerating potential
• Bremsstrahlung radiationprovides smoothbackground
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 5 / 8
X-Ray Tube Spectrum
• Characteristic energy ofelemental fluorescenceemission
• Minimum wavelength(maximum energy) set byaccelerating potential
• Bremsstrahlung radiationprovides smoothbackground
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 5 / 8
Synchrotron Sources
Bending magnet
• Wide horizontal beam
• Broad spectrum to highenergies
Undulator
• Highly collimated beam
• Highly peaked spectrumwith harmonics
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 6 / 8
Synchrotron Sources
Bending magnet
• Wide horizontal beam
• Broad spectrum to highenergies
Undulator
• Highly collimated beam
• Highly peaked spectrumwith harmonics
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 6 / 8
Synchrotron Sources
Bending magnet
• Wide horizontal beam
• Broad spectrum to highenergies
Undulator
• Highly collimated beam
• Highly peaked spectrumwith harmonics
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 6 / 8
Synchrotron Sources
Bending magnet
• Wide horizontal beam
• Broad spectrum to highenergies
Undulator
• Highly collimated beam
• Highly peaked spectrumwith harmonics
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 6 / 8
Synchrotron Sources
Bending magnet
• Wide horizontal beam
• Broad spectrum to highenergies
Undulator
• Highly collimated beam
• Highly peaked spectrumwith harmonics
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 6 / 8
Synchrotron Sources
Bending magnet
• Wide horizontal beam
• Broad spectrum to highenergies
Undulator
• Highly collimated beam
• Highly peaked spectrumwith harmonics
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 6 / 8
Bending Magnet Spectra
0 20000 40000 60000 80000 1e+050
1e+13
2e+13
3e+13
APS
NSLS
ALS
ESRF
Lower energy sources, such as NSLS have lower peak energy and higherintensity at the peak.Higher energy sources, such as APS have higher energy spectrum and areonly off by a factor of 2 intensity at low energy.
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 7 / 8
Bending Magnet Spectra
0 20000 40000 60000 80000 1e+050
1e+13
2e+13
3e+13
APS
NSLS
ALS
ESRF
Lower energy sources, such as NSLS have lower peak energy and higherintensity at the peak.
Higher energy sources, such as APS have higher energy spectrum and areonly off by a factor of 2 intensity at low energy.
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 7 / 8
Bending Magnet Spectra
0 20000 40000 60000 80000 1e+050
1e+13
2e+13
3e+13
APS
NSLS
ALS
ESRF
Lower energy sources, such as NSLS have lower peak energy and higherintensity at the peak.Higher energy sources, such as APS have higher energy spectrum and areonly off by a factor of 2 intensity at low energy.
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 7 / 8
Bending Magnet Spectra
100 1000 10000 1e+051e+05
1e+10
1e+15
APS
NSLS
ALS
ESRF
Logarithmic scale shows clearly how much more energetic and intense thebending magnet sources at the 6 GeV and 7 GeV sources are.
C. Segre (IIT) PHYS 570 - Fall 2010 September 02, 2010 8 / 8