Today’s Outline - January 22, 2015csrri.iit.edu/~segre/phys570/15S/lecture_04.pdfThe Fourier...

Today’s Outline - January 22, 2015

• Bending magnet review

• Insertion devices

• Undulator parameters

• Fundamental wavelength from an undulator

• Higher harmonics

• On and off-axis spectrum

• Undulator to wiggler comparison

Homework Assignment #01:Chapter Chapter 2: 2,3,5,6,8due Thursday, January 29, 2015

C. Segre (IIT) PHYS 570 - Spring 2015 January 22, 2015 1 / 23

Curved arc emission

The observer, looking in the plane of the circulartrajectory,

“sees” the electron oscillate over a halfperiod in a time ∆t (observer’s frame).The electron, in the laboratory frame, travels thisarc in:

∆t ′ =(1/γ)ρ

Because of the Doppler shift, the observer sees theelectron emitting a pulse of radiation of length

∆t ∝ ∆t ′

γ3ωo

The Fourier transform of this pulse is the spectrumof the radiation from the bending magnet.

Curved arc emission

The observer, looking in the plane of the circulartrajectory, “sees” the electron oscillate over a halfperiod

in a time ∆t (observer’s frame).The electron, in the laboratory frame, travels thisarc in:

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

The observer, looking in the plane of the circulartrajectory, “sees” the electron oscillate over a halfperiod in a time ∆t (observer’s frame).

The electron, in the laboratory frame, travels thisarc in:

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

The observer, looking in the plane of the circulartrajectory, “sees” the electron oscillate over a halfperiod in a time ∆t (observer’s frame).The electron, in the laboratory frame, travels thisarc in:

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Curved arc emission

∆t ′ =(1/γ)ρ

∆t ∝ ∆t ′

γ3ωo

Characteristic Energy of a Bending Magnet

The radiation from a bending magnet is defined by it’s characteristicfrequency, ωc which, when the calculation is performed rigorously is:

ωc =3

2γ3ωo

but since T is the period of the rotation through the full circle of radius ρ

ωo =2π

T= 2π

2πρ=

we can therefore calculate the characteristic energy Ec

Ec = ~ωc =3

(mc2)2

converting to storage ring units

Ec [keV] = 0.665E2[GeV]B[T]

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

= 2πc

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

ωc =3

2γ3ωo

ωo =2π

T= 2π

2πρ=

Ec = ~ωc =3

(mc2)2

Bending magnet spectrum

When the radiation pulse time isFourier transformed, we obtainthe spectrum of a bendingmagnet.

Scaling by the characteristicenergy, gives a universal curve

1.33×1013E2 I(ω

K 22/3

)where K2/3 is a modified Besselfunction of the second kind.

0 20 40 60 80 100Photon Energy (keV)

7.0 GeV

6.0 GeV

2.6 GeV

1.9 GeV 1.3 T

1.33×1013E2 I(ω

K 22/3

0 20 40 60 80 100Photon Energy (keV)

7.0 GeV

6.0 GeV

2.6 GeV

1.9 GeV 1.3 T

1.33×1013E2 I(ω

K 22/3

0 2 4 6 8 10E/E

3.1 keV

5.4 keV

19.2 keV

19.4 keV

1.33×1013E2 I(ω

K 22/3

)where K2/3 is a modified Besselfunction of the second kind. 0 2 4 6 8 10

3.1 keV

5.4 keV

19.2 keV

19.4 keV

Power from a bending magnet

The radiated power is given in storage ring units by:

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

where L is the length of the arc visible to the observer and I is the storagering current.We can calculate this for the ESRF where E = 6 GeV, B = 0.8 T,Ec = 19.2 keV and the bending radius ρ = 24.8 m. Assuming that theaperture is 1 mm2 at a distance of 20 m, the angular aperture is1/20 = 0.05 mrad and the flux at the characteristic energy is given by:

Flux = (1.95×1013)(0.052mrad2)(62GeV2)(0.2A) = 3.5×1011ph/s/0.1%BW

The arc length is L = (24.8m)(0.05mrad) = 1.24mm and we have:

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

where L is the length of the arc visible to the observer and I is the storagering current.

We can calculate this for the ESRF where E = 6 GeV, B = 0.8 T,Ec = 19.2 keV and the bending radius ρ = 24.8 m. Assuming that theaperture is 1 mm2 at a distance of 20 m, the angular aperture is1/20 = 0.05 mrad and the flux at the characteristic energy is given by:

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

Flux = (1.95×1013)

(0.052mrad2)(62GeV2)(0.2A) = 3.5×1011ph/s/0.1%BW

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

Flux = (1.95×1013)(0.052mrad2)

(62GeV2)(0.2A) = 3.5×1011ph/s/0.1%BW

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

Flux = (1.95×1013)(0.052mrad2)(62GeV2)

(0.2A) = 3.5×1011ph/s/0.1%BW

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

Flux = (1.95×1013)(0.052mrad2)(62GeV2)(0.2A)

= 3.5×1011ph/s/0.1%BW

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2

(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2

(1.24× 10−3m)(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)

(0.2A) = 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A)

= 7.3W

P[kW] = 1.266E2[GeV]B2[T]L[m]I [A]

P = 1.266(6GeV)2(0.8T)2(1.24× 10−3m)(0.2A) = 7.3W

Polarization

A bending magnet also produces circularly polarized radiation

• If the observer is in the plane of theelectron orbit, the electron motionlooks like a half period of linearsinusoidal motion

• From above, the motion looks like anarc in the clockwise direction

• From below, the motion looks like anarc in the counterclockwise direction

The result is circularly polarized radiation above and below the on-axisradiation.

Polarization

Wigglers and undulators

Wiggler

Like bending magnet except:

• larger ~B → higher Ec

• more bends → higher power

Undulator

Different from bending magnet:

• shallow bends → smaller source

• interference → peaked spectrum

Wiggler

Undulator

Wiggler

Undulator

Wiggler

Undulator

Wiggler

Undulator

Wiggler

Undulator

Wiggler

Undulator

Wiggler

Undulator

Wiggler radiation

• The electron’s trajectory through a wiggler can be considered as aseries of short circular arcs, each like a bending magnet

• If there are N poles to the wiggler, there are 2N arcs

• Each arc contributes as might a single bending magnet but the morelinear path means that the effective length, L, is much longer.

• The magnetic field varies along the length of the wiggler and is higherthan that in a bending magnet, having an average value ofBrms = Bo/

• This results in a significantly higher power load on all downstreamcomponents

Power [kW] = 1.266E2e [GeV]B2[T]L[m]I [A]

Wiggler radiation

Power [kW] = 0.633E2e [GeV]B2o [T]L[m]I [A]

Wiggler radiation

Power [kW] = 0.633E2e [GeV]B2o [T]L[m]I [A]

Undulator characterization

Undulator radiation is characterized bythree parameters:

• The energy of the electrons, γmc2

• The wavelength, λu = 2π/ku, ofit’s magnetic field

• The maximum angular deviaton ofthe electron, αmax

From the electron trajectory:

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku cos (kuz)∣∣∣z=0

= Aku = 2πA/λu

Define a dimensionless quantity, K which scales αmax to the naturalopening angle of the radiation, 1/γ

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

x = A sin (kuz)

αmax =dx

∣∣∣z=0

= Aku = 2πA/λu

K = αmaxγ

Circular path approximation

Consider the trajectory of the electron along one period of the undulator.

Since the curvature is small, the path can be approximated by an arc or acircle of radius ρ whose origin lies at x = −(ρ− A) and z = 0.The equation of the circle which approximates the arc is:

ρ2 = [x + (ρ− A)]2 + z2

x + (ρ− A) =√ρ2 − z2

Consider the trajectory of the electron along one period of the undulator.Since the curvature is small, the path can be approximated by an arc or acircle of radius ρ whose origin lies at x = −(ρ− A) and z = 0.

The equation of the circle which approximates the arc is:

ρ2 = [x + (ρ− A)]2 + z2

x + (ρ− A) =√ρ2 − z2

Consider the trajectory of the electron along one period of the undulator.Since the curvature is small, the path can be approximated by an arc or acircle of radius ρ whose origin lies at x = −(ρ− A) and z = 0.The equation of the circle which approximates the arc is:

ρ2 = [x + (ρ− A)]2 + z2

x + (ρ− A) =√ρ2 − z2

ρ2 = [x + (ρ− A)]2 + z2

x + (ρ− A) =√ρ2 − z2

ρ2 = [x + (ρ− A)]2 + z2

x + (ρ− A) =√ρ2 − z2

Radius of curvature

From the equation for a circle:

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

For the undulating path:

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

≈ A− Ak2uz2

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u

−→ ρ =1

λ2u4π2A

Radius of curvature

x = A− ρ+√ρ2 − z2

= A− ρ+ ρ

√1− z2

≈ A− ρ+ ρ

(1− 1

)≈ A− z2

x = A cos (kuz)

(1− k2uz

)≈ A− Ak2uz

Combining, we have

Ak2uz2

2−→ 1

ρ= Ak2u −→ ρ =

λ2u4π2A

Electron path length

The displacement ds of the elec-tron can be expressed in terms ofthe two coordinates, x and z as:

ds =√

(dx)2 + (dz)2

√1 +

dzA cos kuz = −Aku sin kuz

Now calculate the length of the path traveled by the electron over oneperiod of the undulator

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

dzA cos kuz

= −Aku sin kuz

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

ds =√

(dx)2 + (dz)2

√1 +

Sλu =

∫ λu

√1 +

dz ≈∫ λu

∫ λu

A2k2u2

sin2 kuz

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

)= λu

Using the identity:

sin2 kuz =1 + cos 2kuz

integrating, the finalterm vanishes

using the definition ofthe undulator parameter,K = γAku, we have

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

)= λu

Using the identity:

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

)= λu

Using the identity:

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

)= λu

Using the identity:

integrating,

the finalterm vanishes

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

)= λu

Using the identity:

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

Using the identity:

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

Using the identity:

Sλu =

∫ λu

A2k2u2

sin2 kuz

∫ λu

A2k2u2

2− 1

2cos 2kuz

A2k2u4

z +A2ku

8sin 2kuz

∣∣∣∣λu0

A2k2u4

)= λu

Using the identity:

The K parameter

Given the definition K = γAku, we can rewrite the radius of curvature ofthe electron’s path in the undulator as

Ak2u−→ ρ =

Recalling that the radius of curvature is related to the electron momentumby the Lorentz force, we have

p = γmv ≈ γmc = ρeBo −→ γmc ≈ γ

KkueBo

Combining the above expressions yields

K =eBo

2πmcλuBo = 0.934λu[cm]Bo [T]

For APS Undulator A, λu = 3.3cm and Bo = 0.6T at closed gap, so

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

−→ ρ =γ

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

p = γmv

≈ γmc = ρeBo −→ γmc ≈ γ

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

p = γmv ≈ γmc

= ρeBo −→ γmc ≈ γ

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

p = γmv ≈ γmc = ρeBo

−→ γmc ≈ γ

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

2πmcλuBo

= 0.934λu[cm]Bo [T]

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T]

= 1.85

The K parameter

Ak2u−→ ρ =

KkueBo

K =eBo

K = 0.934 · 3.3[cm] · 0.6[T] = 1.85

Undulator wavelength

Consider an electron traveling through the undulator and emittingradiation at the first maximum excursion from the center.

The emitted wave travels slightlyfaster than the electron.It moves cT ′ in the time the elec-tron travels a distance λu along theundulator.

The observer sees radiation with acompressed wavelength, along withharmonics which satisfy the samecondition.

nλn = cT ′ − λu

The emitted wave travels slightlyfaster than the electron.

It moves cT ′ in the time the elec-tron travels a distance λu along theundulator.

The observer sees radiation with acompressed wavelength,

along withharmonics which satisfy the samecondition.

= cT ′ − λu

The observer sees radiation with acompressed wavelength,

along withharmonics which satisfy the samecondition.

λ1 = cT ′ − λu

The fundamental wavelength

The fundamental wavelength must becorrected for the observer angle θ

λ1 = cT ′ − λu cos θ

v− cos θ

β− cos θ

Over the time T ′ the electronactually travels a distance Sλu,so that

T ′ =Sλuv

S ≈ 1 +K 2

Since γ is large, the maximum observation angle θ is small so

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

=λu2γ2

2β− 2γ2 + γ2θ2

v− cos θ

β− cos θ

T ′ =Sλuv

S ≈ 1 +K 2

λ1 ≈ λu(

4γ2β− 1 +

λu2γ2

2β− 2γ2 + γ2θ2

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

λ1 ≈λu2γ2

2β− 2γ2 + γ2θ2

≈ λu2γ2

β− 1

2β− (γθ)2

≈ λu2γ2

1− β2

[1− ββ

2β− (γθ)2

≈ λu2γ2

β(1 + β)+

2β− [γθ]2

regrouping terms

1− β2

1− β2 = (1 + β)(1− β)

If we assume that β ∼ 1 for these highly relativistic electrons

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

≈ λu2γ2

2β− (γθ)2

)and directly on axis

λ1 ≈λu2γ2

)for a typical undulator γ ∼ 104, K ∼ 1, and λu ∼ 2cm so we estimate

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

This corresponds to an energy E1 ≈ 8.2keV but as the undulator gap iswidened, Bo decreases, K decreases, λ1 decreases, and E1 increases.

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

≈ λu2γ2

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

and directly on axis

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

for a typical undulator γ ∼ 104, K ∼ 1, and λu ∼ 2cm so we estimate

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

= 1.5× 10−10m = 1.5A

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

This corresponds to an energy E1 ≈ 8.2keV but as the undulator gap iswidened

, Bo decreases, K decreases, λ1 decreases, and E1 increases.

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

This corresponds to an energy E1 ≈ 8.2keV but as the undulator gap iswidened, Bo decreases

, K decreases, λ1 decreases, and E1 increases.

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

This corresponds to an energy E1 ≈ 8.2keV but as the undulator gap iswidened, Bo decreases, K decreases

, λ1 decreases, and E1 increases.

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

This corresponds to an energy E1 ≈ 8.2keV but as the undulator gap iswidened, Bo decreases, K decreases, λ1 decreases

, and E1 increases.

λ1 ≈λu2γ2

β(1 + β)+

2β− (γθ)2

)≈ λu

2β− (γθ)2

λ1 ≈λu2γ2

λ1 ≈2× 10−2

2 (104)2

)= 1.5× 10−10m = 1.5A

Higher harmonics

dt ′= 1− ~n · ~β(t ′)

≈ 1− β[αφ+

(1− θ2

2− α2

Recall that we developed an expres-sion for the Doppler time compres-sion of the emission from a movingelectron as a function of the ob-server angle.

This can be rewritten in terms ofthe coordinates in the figure usingthe vector of unit length in the ob-server direction:

~n ≈{φ, ψ, (1− θ2/2)

}~β ≈ β

{α, 0, (1− α2/2)

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

Higher harmonics

dt ′= 1− ~n · ~β(t ′)

≈ 1− β[αφ+

(1− θ2

2− α2

Recall that we developed an expres-sion for the Doppler time compres-sion of the emission from a movingelectron as a function of the ob-server angle.

This can be rewritten in terms ofthe coordinates in the figure usingthe vector of unit length in the ob-server direction:

~n ≈{φ, ψ, (1− θ2/2)

}~β ≈ β

{α, 0, (1− α2/2)

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

Higher harmonics

dt ′= 1− ~n · ~β(t ′)

≈ 1− β[αφ+

(1− θ2

2− α2

Recall that we developed an expres-sion for the Doppler time compres-sion of the emission from a movingelectron as a function of the ob-server angle.This can be rewritten in terms ofthe coordinates in the figure usingthe vector of unit length in the ob-server direction:

~n ={φ, ψ,

√1− θ2

}~β = β

{α, 0,

√1− α2

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

Higher harmonics

dt ′= 1− ~n · ~β(t ′)

≈ 1− β[αφ+

(1− θ2

2− α2

~n ≈{φ, ψ, (1− θ2/2)

}~β ≈ β

{α, 0, (1− α2/2)

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

Higher harmonics

dt ′= 1− ~n · ~β(t ′)

≈ 1− β[αφ+

(1− θ2

2− α2

~n ≈{φ, ψ, (1− θ2/2)

}~β ≈ β

{α, 0, (1− α2/2)

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

Higher harmonics

dt ′= 1− ~n · ~β(t ′)

≈ 1− β[αφ+

(1− θ2

2− α2

~n ≈{φ, ψ, (1− θ2/2)

}~β ≈ β

{α, 0, (1− α2/2)

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)C. Segre (IIT) PHYS 570 - Spring 2015 January 22, 2015 19 / 23

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

≈ 1− 1− αφ+θ2

(θ2 + α2 +

)− αφ

This differential equation can be solved, realizing that φ and θ areconstant while α(t ′) varies as the electron moves through the insertiondevice, and gives:

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

ω1 � ωu as expected because of the Doppler compression , but they arenot proportional because of the second and third terms.

The motion of the electron, sinωut′, is always sinusoidal, but because of

the additional terms, the motion as seen by the observer, sinω1t, is not.

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′

− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

ω1 � ωu as expected because of the Doppler compression

, but they arenot proportional because of the second and third terms.

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

ω1 � ωu as expected because of the Doppler compression , but they arenot proportional because of the second

and third terms.

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

Higher harmonics

dt ′≈ 1−

(1− 1

)(1 + αφ− θ2

2− α2

)≈ 1− 1− αφ+

(θ2 + α2 +

)− αφ

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

the additional terms, the motion as seen by the observer, sinω1t, is not.C. Segre (IIT) PHYS 570 - Spring 2015 January 22, 2015 20 / 23

On-axis undulator characteristics

ω1t = ωut′ − K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

Suppose we have K = 1 and θ = 0(on axis), then

ω1t = ωut′ +

6sin (2ωut

Plotting sinωut′ and sinω1t shows

the deviation from sinusoidal.

Similarly, for K = 2 and K =5, the deviation becomes more pro-nounced. This shows how higherharmonics must be present in the ra-diation as seen by the observer. 0 π/2 π

Phase Angle (radians)

pure sine

on axis

ω1t = ωut′ − K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

ω1t = ωut′ +

6sin (2ωut

Similarly, for K = 2 and K =5, the deviation becomes more pro-nounced. This shows how higherharmonics must be present in the ra-diation as seen by the observer. 0 π/2 π

pure sine

on axis

ω1t = ωut′ − K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

ω1t = ωut′ +

6sin (2ωut

Similarly, for K = 2 and K =5, the deviation becomes more pro-nounced. This shows how higherharmonics must be present in the ra-diation as seen by the observer.

0 π/2 π

pure sine

on axis

ω1t = ωut′ − K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

ω1t = ωut′ +

6sin (2ωut

Similarly, for K = 2

and K =5, the deviation becomes more pro-nounced. This shows how higherharmonics must be present in the ra-diation as seen by the observer.

0 π/2 π

pure sine

on axis

ω1t = ωut′ − K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

ω1t = ωut′ +

6sin (2ωut

Similarly, for K = 2 and K =5, the deviation becomes more pro-nounced.

This shows how higherharmonics must be present in the ra-diation as seen by the observer.

0 π/2 π

pure sine

on axis

ω1t = ωut′ − K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

ω1t = ωut′ +

6sin (2ωut

Similarly, for K = 2 and K =5, the deviation becomes more pro-nounced. This shows how higherharmonics must be present in the ra-diation as seen by the observer. E 3E 5E

Energy

nsity (

. units)

pure sine

Off-axis undulator characteristics

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

0 π/2 π

ctional D

φ=θ=1/γ

When K = 2 and θ = φ = 1/γ, wehave

ω1t = ωut′+

4sin (2ωut

′) + sinωut′

The last term introduces an antisym-metric term which skews the func-tion and leads to the presence offorbidden harmonics (2nd , 4th, etc)in the radiation from the undulatorcompared to the on-axis radiation.

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

0 π/2 π

ctional D

φ=θ=1/γ

ω1t = ωut′+

4sin (2ωut

′) + sinωut′

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

0 π/2 π

φ=θ=1/γ

ω1t = ωut′+

4sin (2ωut

′) + sinωut′

The last term introduces an antisym-metric term which skews the func-tion

and leads to the presence offorbidden harmonics (2nd , 4th, etc)in the radiation from the undulatorcompared to the on-axis radiation.

ω1t = ωut′− K 2/4

1 + (γθ)2 + K 2/2sin (2ωut

′)− 2Kγ

1 + (γθ)2 + K 2/2φ sin (ωut

E 3E 5E

Energy

nsity (

. units)

K=1 θ=0

K=1 φ=θ=1/γ

K=5 φ=θ=1/γ

even harmonics

ω1t = ωut′+

4sin (2ωut

′) + sinωut′

Spectral comparison

• Brilliance is 6 orders largerthan a bending magnet

• Both odd and evenharmonics appear

• Harmonics can be tuned inenergy (dashed lines)

Spectral comparison

Today’s Outline - January 22, 2015csrri.iit.edu/~segre/phys570/15S/lecture_04.pdfThe Fourier...

Documents

Structure and melting of Bi nanocrystals embedded in a B2O3-Na2O …csrri.iit.edu/~segre/phys570/13F/presentations/siqueira.pdf · PHYS 570 -Introduction to Synchrotron Radiation

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

Today’s Outline - October 19, 2016csrri.iit.edu/~segre/phys570/16F/lecture_16.pdf · Today’s Outline - October 19, 2016 Final presentation Ewald sphere (continued) Modulated Structures

Sulfidation Processes of PVP-Coated Silver Nanoparticles ...csrri.iit.edu/~segre/phys570/15S/presentations/moazzen.pdf · Sulfidation Processes of PVP-Coated Silver Nanoparticles

In-situ and operando XAFS studies of fuel cell catalystscsrri.iit.edu/~segre/phys570/13F/lecture_19.pdfIn-situ and operando XAFS studies of fuel cell catalysts Carlo Segre Physics

Illinois Institute of Technology PHYS-570 Introduction to ...csrri.iit.edu/~segre/phys570/15S/presentations/kucuk.pdf · Final Presentation: Kamil KUCUK-A20306046 Prof. Dr. Carlo

Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates

Today’s Outline - August 31, 2016csrri.iit.edu/~segre/phys570/16F/lecture_04.pdf · The light pulse emitted at B is therefore, a distance(c v cos ) t0 behind the pulse emitted at

csrri.iit.educsrri.iit.edu/~segre/phys570/12S/lecture_05.pdf · Today’s Outline - January 24, 2012 Starting with a parameterization of the electron path through an undulator, we

Physics 570 Michael Martynowycz - Illinois Institute of ...csrri.iit.edu/~segre/phys570/12S/presentations/martynowycz.pdf · Michael Martynowycz . The Structural Basis for Specificity

Today’s Outline - February 19, 2015csrri.iit.edu/~segre/phys570/15S/lecture_10.pdfToday’s Outline - February 19, 2015 Homework #2 solutions Refractive optics Research papers Homework

Today’s Outline - November 16, 2016csrri.iit.edu/~segre/phys570/16F/lecture_23.pdf · Today’s Outline - November 16, 2016 Resonant and inelastic techniques Di raction anomalous

PHYS 570 - Introduction to Synchrotron Radiationcsrri.iit.edu/~segre/phys570/15S/lecture_01.pdfPHYS 570 - Introduction to Synchrotron Radiation Term: Spring 2015 Meetings: Tuesday

Illinois Institute of Technology PHYS-570 Introduction to ...phys.iit.edu/~segre/phys570/15S/presentations/kucuk.pdf · Final Presentation: Kamil KUCUK-A20306046 Prof. Dr. Carlo U

Today’s Outline - September 18, 2013csrri.iit.edu/~segre/phys570/13F/lecture_09.pdf · Today’s Outline - September 18, 2013 Models of Surfaces Re ectivity from the MRCAT mirror

Today’s Outline - September 19, 2016csrri.iit.edu/~segre/phys570/16F/lecture_08.pdf · Today’s Outline - September 19, 2016 Re ection from a thin slab Kiessig fringes Kinematical

Today’s Outline - January 23, 2018phys.iit.edu/~segre/phys570/18S/lecture_05.pdf · Today’s Outline - January 23, 2018 Fundamental wavelength from an undulator Higher harmonics

phys.iit.eduphys.iit.edu/~segre/phys570/16F/lecture_04.pdf · O -axis emission A B C v cosa Dt' cDt' a (c-vcosa)Dt' Consider the emission from seg-ment AB, which is not along the

Longitudinal Coherence - Synchrotron Radiation …csrri.iit.edu/~segre/phys570/10F/lecture_04.pdf · Longitudinal Coherence De nition: Distance over which two waves from the same

Today’s Outline - October 17, 2016csrri.iit.edu/~segre/phys570/16F/lecture_15.pdfC. Segre (IIT) PHYS 570 - Fall 2016 October 17, 2016 1 / 19 Today’s Outline - October 17, 2016