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Low energy beamline on the new

Storage Ring at MAX-lab

Sverker Werin

MAX-lab

2011-11-09





The aim has been to optimise the radiation from an insertion device in the

wavelength region 5-40 eV and to see how the new 600-700 MeV storage ring

performs relative to MAX II.



A number of type set ups have been analysed at 4, 25 and 40 eV giving the result

that:



 The new ring is superior at 4 eV, slightly better at 25, while MAX II is better at

40 eV (and most likely beyond).

 At 40 eV the radiation from MAX II has a higher peak flux, while there is no

difference at lower energies.

 MAX II gives a significantly higher total power within the acceptance. At 5 eV

up to 200 W.



Table 1. A set of different devices at MAX-lab



Period N Kmax Bmax Gap

MAX II 1.5 GeV 0.1 m 25 10.76 1.15 T 22 mm

MAX B 600 MeV 0.066 m 30 4.40 0.713 T 22 mm

MAX B 700 MeV 0.07 m 28 5.04 0.771 T 22 mm





Model

The radiation of interest here is the radiation that comes to the monochromator

within the physical aperture (entrance slit, acceptance...) and within the energy

resolution (energy window) of the monochromator.



The energy resolution is 1/10.000 which means an energy window with E =

E/10.000. For all practical purposes this window is much smaller than all effects

present in the undulator radiation. We can thus assume that all broadening effects

comes from the undulator and that the radiation across the energy window is

constant.



The radiation coming to a point, p, on the entrance aperture (Figure 1) of the

monochromator has a certain centre energy, EU., different from the energy at the

very centre of the radiation cone: EU .

EU U   .



The linewidth at this point, p, is given by contributions from energy spread, the

natural linewidth, beam divergence (and possibly the beamsize), errors in the

undulator.

Let us here neglect the contributions from the beamsize and errors in the

undulator.

The linewidth from the undulator is more or less constant over the emission angles,

and we assume that the same linewidth is present at all points on the aperture.

Both the energy of the

centre point and the

intensity varies with the p

distance to the cone 

centre.



The intensity at point p at

the energy of the energy

window in the

monochromator, Em, can

be extracted from the

linewidth and the distance E E EU

m U 0

from the centre energy at

point p.

E U  m 

Figure 1. Layout



The energy varies like :

1,24  106 1,24  106

EeV  6,24  1018

hc

  .

 w  K 2 2 2

w 2

1        

2i 2 

 2 

 2i



As EU moves with  we can translate the energy intensity distribution to an angular

intensity distribution.



Example:

Lets choose an "ideal case" when Em = EU0 (The monochromator tuned to

the peak of the undulator spectrum), and an optimum opening angle when

the intensity has dropped to 50 % value at EU0. This occurs at the HWHM

point of the linewidth.



The natural linewidth of a 25 pieces of 0.1 m period undulator at first

harmonic is 1/25 = 0.04 (FWHM), and thus the HWHM is at 0.02.

  2 2



 K2

1

2

which for:K= 5; = 3000 translates into: =0.17 mRad.



In reality the linewidth is larger due

to additional broadening effects. 10 mm MPW on MAX II at 40 eV

4,5E-2

4,0E-2 Natural

When do other broadening 3,5E-2 Divergence

effects come into play? Energy

Relative linewidth









3,0E-2

Total

2,5E-2

Braodening effects that come inte play are

2,0E-2

due to: undulator periods (natural energy

spread), e-beam divergence, energy 1,5E-2

spread and magnetic imperfections in the 1,0E-2

undulator. The last effect is normally

50,0E-4

neglectable. These effects add up to a

total linewidth. 00,0E+0

0 2 4 6 8

Harmonic (i)

In figure 2 there are the linewidths for a 10

mm period undulator on MAX II. We can Figure 2. Linwidths of a 10 mm undulator on MAX II.







2

see that operation at a low harmonic (here at fixed energy) gives a linewidth

dominated by the natural linewidth. While moving up in harmonics the linewidth

changes to be energy spread dominated.

At the first harmonic it is perfectly enough to

New ring, 66 mm Undulator at 25 eV only include the natural energy spread.

3,5E-2

Natural The other example is the 66 mm period

3,0E-2

Divergence undulator on the new ring (figure 3), where

2,5E-2 the situation is very similar to the 10 mm

Realtive linewidth









Energy

Total case on MAX II.

2,0E-2



1,5E-2 One point here is that to do simulations

1,0E-2

including energy spread is difficult as the

standard codes to not include this effect.

50,0E-4



00,0E+0 By only regarding cases using harmonic 3 or

0 1 2 3 4 5 6 lower it is not too bad to neglect the effect of

harmonic (i) energy spread.

Figure 3. Linewidths of an undulator on the new ring.







Results

The results from the simulations are given in the tables on the coming pages. All

important values are within a factor of 3 from each other, except the total power

inside the aperture which is significantly higher for devices utilising MAX II.



The opening angles have been chosen "by eye" to suit the emission cones

resulting from the program. In the same way the "Not On Top" values, which

means that the monochromator has been tuned away from the wavelength of the

undulator peak, to take advantage of a larger integrated flux over the aperture for

these cases, have been chosen "by eye". (figure 4).

Figure 4 a-c. Flux through different opening angles. 30 period, 0.066 m undulator

on the new ring at 25 eV. c) not on top.







20E+14

18E+14

16E+14

14E+14

12E+14

Flux 10E+14

8E+14

6E+14

4E+14

2E+14 0,2

8

00E+0 -0 , mRad

03

5

-0 0

10

5









-0 ,

70

,3









0







35

,2









0

07

-0







,0







21





0

-0









35

0,



0,



0,





mRad









20E+14

18E+14

16E+14

14E+14

12E+14

Flux 10E+14

8E+14

6E+14

4E+14

2E+14 0,1

4

00E+0 -0 ,

01 mRad

75

-0 5

05

7









-0 ,

35

,1









5









17

,1









5

03

-0







,0









5

10





5

-0









17

0,



0,



0,









mRad









16E+14

14E+14

12E+14

10E+14

Flux 8E+14

6E+14

4E+14

2E+14 0,2

8

00E+0 -0 , mRad

03

5

-0 0

10

5









-0 ,

70

,3









0









35

,2









0

07

-0







,0







21





0

-0









35

0,



0,



0,









mRad









4

5 eV

Device Radiation +-0,35 mRad +-0,6 mRad

Booster SR N=30 4,84 eV 5,16e14 5,16e14 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=4,4 On Top 1,71e12 2,08e13 Flux within aperture (100 mA 1/10.000BW)

L=2m 23 23 Total power (W)

=0.066m 1,47 4,32 Power within aperture (W)

Booster SR N=30 4,78 eV 4,76e14 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=4,4 Not On Top 3,15e13 Flux within aperture (100 mA 1/10.000BW)

L=2m 23 Total power (W)

=0.066m 4,32 Power within aperture (W)

Booster SR N=37 4,84 eV 7,75e14 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=4,4 On Top 2,68e13 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 28 Total power (W)

=0.066m 5,32 Power within aperture (W)

MAX II N=25 4,935 eV 6,7e14 6,7e14 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

1500 MeV K=9,2 On Top 1,42e12 1,50e13 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 345 345 Total power (W)

=0.1m 66,2 194 Power within aperture (W)

MAX II N=25 4,80 eV 5,35e14 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

1500 MeV K=9,2 Not On Top 2,81e13 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 345 Total power (W)

=0.1m 194 Power within aperture (W)









5

25 eV

Device Radiation +- 0,175 mR +- 0,35

mRad

Booster SR N=30 24,25 eV 1,80e15 1.8*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=1,5 On Top 1,43e12 1.95*1013 Flux within aperture (100 mA 1/10.000BW)

L=2m 1st harm 2,67 W 2,67 Total power (W)

=0.066m 0,122 W 0,49 Power within aperture (W)

Booster SR N=30 24.0 eV 1.59*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=1,5 Not On Top 2.58*1013 Flux within aperture (100 mA 1/10.000BW)

L=2m 1st harm 2,67 Total power (W)

=0.066m 0,49 Power within aperture (W)

Booster SR N=37 24,25 eV 2.65*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=1,5 On Top 2.55*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 1st harm 2,67 Total power (W)

=0.066m 0,49 Power within aperture (W)

Booster SR N=37 24.00eV 2.22*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=1,5 Not On Top 3.36*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 1st harm 2.67 Total power (W)

=0.066m 0.49 Power within aperture (W)

MAX II N=25 24,8eV 2.79*1015 2.79*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

1500 MeV K=3,9 On Top 1.47*1012 1.63*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 1st harm 62 62 Total power (W)

=0.1m 7.0 27.9 Power within aperture (W)

MAX II N=25 24,4eV 2.45*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

1500 MeV K=3,9 Not On Top 2.62*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 1st harm 62 Total power (W)

=0.1m 27.9 Power within aperture (W)











6

40 eV

Device Radiation +- 0,125 +- 0.25

Booster SR N=30 40,0eV 1,62*1015 1,62*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=2,4 On Top 0,79*1012 1,09*1013 Flux within aperture (100 mA 1/10.000BW)

L=2m 3rd harm 6,8 6,8 Total power (W)

=0.066m 0,1 0,4 Power within aperture (W)

Booster SR N=30 39,7eV 1,23*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=2,4 Not On Top 1,41*1013 Flux within aperture (100 mA 1/10.000BW)

L=2m 3rd harm 6,8 Total power (W)

=0.066m 0,4 Power within aperture (W)

Booster SR N=37 40,0eV 2,36*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

600 MeV K=2,4 On Top 1,43*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 3rd harm 8,4 Total power (W)

=0.066m 0,5 Power within aperture (W)

Booster SR N=37 39,0eV 1,74*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

700 MeV K=2,85 Not On Top 1,82*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 3rd harm 15,3 Total power (W)

=0.07m 1,04 Power within aperture (W)

MAX II N=25 39,9eV 4,3*1015 4,3*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

1500 MeV K=2,95 On Top 1,55*1012 1,56*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 35,5 35,5 Total power (W)

=0.1m 2,7 10,74 Power within aperture (W)

MAX II N=25 39,3eV 3,83*1015 Peak angular flux density (ph/(s mr^2 100mA 0.1%BW)

1500 MeV K=2,95 Not On Top 2,51*1013 Flux within aperture (100 mA 1/10.000BW)

L=2,5m 35,5 Total power (W)

=0.1m 10,74 Power within aperture (W)











7



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