beutner - bunch compression experiment in vuv-fel bc3 filebunch compression experiment in vuv-fel...

Bolko BeutnerBeam Dynamics Meeting3.4.2006

Bunch Compression Experiment in VUV-FEL BC3

Overview

IntroductionSimulation MethodsBeam Dynamics in BC3Beam Transport to LOLAProposed Experiment

Introduction

Coherent Synchrotron Radiation in the Bunch Compressors distort the Beam.

Our Goal is to use LOLA to observe CSR effects on the beam.

Both CSR and SpCh forces contribute to the final Beam which makes a clear identification of CSR effects difficult.

Introduction

Furthermore bunch compression in both compressors leads to complicated particle distributions.

To keep the situation as simple as possible we decided to use only one Bunch Compressor (BC3).

M. Dohlus

Simulation Methods

ASTRA ASTRA ASTRA

CSRTrack CSRTrack

ACC1 : on crest

ACC23 : (maximum Compression ~ -28deg)-40deg/-35deg/-30deg/-25deg/0deg

BC3: R = 5.3 malpha = 5.4 deg R56=-0.099369

CSRTrack calculations using‘projected’ method.

1nC and 2nC Bunches

Beam Dynamics in BC3

0deg 2nC -25deg 2nC


-30deg 2nC -35deg 2nC


-40deg 1nC -40deg 2nC

The clearest Signal is the horizontal Displacement

Beam Dynamics in BC3 0deg

longitudinal [m]

horri

zont

al [m

]

Top View with Current profile

-4 -3 -2 -1 0 1 2

x 10-3

-2

-1

0

1

2x 10-3

longitudinal [m]

horri

zont

al [m

]

Top View with centroid curve and width

-4 -3 -2 -1 0 1 2

x 10-3

-2

-1

0

1

2x 10-3

Red solid : Centroid Green dashed : slice width

2nC



2nC

longitudinal [m]

horri

zont

al [m

]


-8 -7 -6 -5 -4 -3 -2 -1 0

x 10-4

-2

-1

0

1

2x 10-3

longitudinal [m]

horri

zont

al [m

]


-8 -7 -6 -5 -4 -3 -2 -1 0

x 10-4

-2

-1

0

1

2x 10-3



2nC

longitudinal [m]

horri

zont

al [m

]


-10 -8 -6 -4 -2 0 2

x 10-4

-2

-1

0

1

2

x 10-3

longitudinal [m]

horri

zont

al [m

]


-10 -8 -6 -4 -2 0 2

x 10-4

-2

-1

0

1

2

x 10-3

Beam Dynamics in BC3 35 deg

longitudinal [m]

horri

zont

al [m

]


-2 -1.5 -1 -0.5 0 0.5 1

x 10-3

-2

0

2x 10-3

longitudinal [m]

horri

zont

al [m

]


-2 -1.5 -1 -0.5 0 0.5 1

x 10-3

-2

0

2x 10-3


2nC


2nC1nC


longitudinal [m]

horri

zont

al [m

]


-3 -2 -1 0 1 2

x 10-3

-3

-2

-1

0

1

x 10-3

longitudinal [m]

horri

zont

al [m

]


-3 -2 -1 0 1 2

x 10-3

-3

-2

-1

0

1

x 10-3

longitudinal [m]

horri

zont

al [m

]


-3 -2 -1 0 1 2

x 10-3

-2

0

2

x 10-3

longitudinal [m]ho

rrizo

ntal

[m]


-3 -2 -1 0 1 2

x 10-3

-2

0

2

x 10-3


-4 -3 -2 -1 0 1 2 3

x 10-3

-1

-0.5

0

0.5

1

1.5

2

2.5

3

3.5x 10-3

longitudinal [m]

hor.

disp

lace

men

t [m

]

centroid curve after bc3

0°40°35°30°25°

Summary of the Centroid curves after BC3


In order to “neglect” space charge forces behind the bunch compressor we focus now on the -40deg case.

In this case the bunch length is the same before and after BC3 (1.53mm). This makes it easy to compare with the on crest case.


The main contribution from CSR forces are in the area of the 3rd Dipole.

Max peak current is about 6kA (2nC).

-2 0 2 4 6 8 10 12 14 160

0.5

1

1.5

2x 10-3

Bun

ch L

engt

h [m

]

Beamline Position [m]-2 0 2 4 6 8 10 12 14 16

0.0176

0.0178

0.018

0.0182

0.0184

Ene

rgy

Spr

ead

[rel.]

Beamline Position [m]

-2 0 2 4 6 8 10 12 14 160

20

40

60

Hor

izon

tal B

eta

Fkt.

[m]

Beamline Position [m]-2 0 2 4 6 8 10 12 14 16

0

0.5

1

1.5x 10-5

Hor

izon

tal E

mitt

ance

[m]

Beamline Position [m]


Evolution of the centroidcurve and the slice rmswidth in BC3.

Dispersion is Substracted.

Red and green lines show the positions of the dipoles.

-4 -3 -2 -1 0 1 2 3

x 10-3

0

1

2

3

4

5

6

7x 10

-3

longitudinal [m]

hor.

disp

lace

men

t [m

]

2nC centroid curve with dispersion compensation

-4 -3 -2 -1 0 1 2 3

x 10-3

0

1

2

3

4

5

6x 10-3

longitudinal [m]

slic

e w

idth

[m]

2nC centroid curve with dispersion compensation

Beam Transport to LOLA

Beam Transport from BC3 to LOLA with ASTRA using Op1 8.8.2005 optics.

Only small longitudinal alterations from space charge forces are expected.

However the optics should have an strong impact on the horizontal centroid curve.


No SpCh 2nC SpCh 2nCAlmost no difference….


No SpCh 1nC SpCh 1nCAlmost no difference….

Beam at LOLA 2nC

longitudinal [m]

horri

zont

al [m

]


-4 -3 -2 -1 0 1 2

x 10-3

-0.02

0

0.02

0.04

longitudinal [m]

horri

zont

al [m

]


-4 -3 -2 -1 0 1 2

x 10-3

-0.02

0

0.02

0.04

longitudinal [m]

horri

zont

al [m

]


-3 -2 -1 0 1 2 3

x 10-3

-0.05

0

0.05

longitudinal [m]ho

rrizo

ntal

[m]


-3 -2 -1 0 1 2 3

x 10-3

-0.05

0

0.05

0deg -40deg

Beam at LOLA 1nC

longitudinal [m]

horri

zont

al [m

]


-4 -3 -2 -1 0 1 2

x 10-3

-0.02

0

0.02

0.04

longitudinal [m]

horri

zont

al [m

]


-4 -3 -2 -1 0 1 2

x 10-3

-0.02

0

0.02

0.04

0deg -40deg

longitudinal [m]

horri

zont

al [m

]


-3 -2 -1 0 1 2

x 10-3

-0.02

0

0.02

0.04

longitudinal [m]ho

rrizo

ntal

[m]


-3 -2 -1 0 1 2

x 10-3

-0.02

0

0.02

0.04

Proposed Experiment

Machine Set Up

Energy after ACC1 = 125 MeVPhase of ACC1 = 0deg (on crest)Energy after ACC23= 380 MeV (on crest)Phases of ACC23 = 0/25/30/35/40deg

Proposed Experiment

Set up machineLOLA measurement

If necessary optics and orbit adjustmentsLOLA pictures at different phases (0/25/30/35/40deg) and charges (0.5/1/2nC)

Optics measurement between BC3 and LOLA for proper tracking of the horizontal centroid curve.

Summary

LOLA should see clear CSR effects on the centroid.In the 2nC case slice energy spread growth from CSR should be observable.In the -40deg case space charge contributions are almost negligible.

beutner - bunch compression experiment in vuv-fel bc3 filebunch compression experiment in vuv-fel...

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