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US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States Particle Accelerator School Dept. of Physics, MIT

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Page 1: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Unit 8 - Lecture 17

Building blocks of storage rings

William A. Barletta

Director, United States Particle Accelerator School

Dept. of Physics, MIT

Page 2: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

In practical units

Dipole magnets to bend the beam

Itotal (Amp turns) =1

0.4B (Gauss) G(cm)

1m 1[ ] = 0.2998

Bo T[ ]

relE GeV[ ]

Ldipole= bend

Page 3: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Quadrupoles to focus the beam

For a Quadrupole with length l & with gradient B'

x Focal point

f

For Z =1 k m 2[ ] = 0.2998 B T /m[ ]

E GeV[ ]k

=q

E B xl

=

R

B T

m

= 2.51

NI [A - turns]

R [mm2]

Page 4: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

BEAM OPTICS screen

Page 5: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Magnet input screens

Page 6: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

FODO transport channel

For stability sinµ

2=

L

2 f f > L /2

FODO cell

-ff/2 f/2

LL

Page 7: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

FODO transport

The (symmetric) FODO transport matrix is

Where

Let = f / L

MFODO = 1 2

L2

f 2 2L 1+L

f

1f * 1 2

L2

f 2

= cos sin

1cos

1

f * = 2 1 Lf

L

f 2

and = betatron phase advance

cos =1 2L2

f 2 =2 2

2 or sin2

=1

Page 8: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

More generally for a lens of finite length

The solution is that of a simple harmonic oscillator

For K < 0 the solution is

For the thin lens, let l 0 keeping Kl finite and 1/f

x

x

out

= cos

1

Ksin

Ksin cos

x

x

out

where = K l

x

x

out

= cosh

1

K sinh

K sinh cosh

x

x

out

with = K l

Page 9: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Symmetric FODO cell

Page 10: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Simple FODO cell

Page 11: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

12-fold symmetric 1 GeV FODO ring

Page 12: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

RF for 1 GeV FODO ring

Page 13: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Longitudinal phase space

Page 14: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

The bend magnet can be in the drift:1/12th of 10 GeV DESY ring

Page 15: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

DESY ring parameters

Page 16: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

DESY ring RF

Page 17: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Example of synchrotron complex: ELSA

Page 18: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

ELSA optical functions

Page 19: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Achromatic Transport Cells

Page 20: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Why use achromats?

We may want to deliver the beam to a region with no

residual dispersion (energy dependent orbit displacement)

Interaction regions in colliders

Insertion devices in storage rings

For circulating electron beams we may want a very low

emittance

Synchrotron light sources

We would like many long straight sections

Hence the low-emittance Chasman-Green lattice (1975)

Basis is Double Bend Achromat (Panofsky, 1965)

Page 21: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

Storage ring building blocks:Double Bend Achromat

Page 22: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

12 of the cells make a 2 GeV electron ring

Page 23: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

With a tune in a dangerous position

Page 24: Unit 8 - Lecture 17 Building blocks of storage rings...US Particle Accelerator School Unit 8 - Lecture 17 Building blocks of storage rings William A. Barletta Director, United States

US Particle Accelerator School

The longitudinal phase space is