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John Arthur Mirror effects [email protected] .edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike Pivovaroff

John Arthur Mirror [email protected] June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

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Page 1: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 1

Effects of LCLS X-Ray MirrorsJohn Arthur

Presenting work by Peter Stefan and Mike Pivovaroff

Page 2: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 2

24mm offsetSiC 1.5mrad

SiC 1.5mrad

Offset mirrors in the FEE

FEL radiation reflected (>95%)

Background from high harmonics and Bremsstrahlung not reflected

Upstream of all LCLS experimentsWill remove high-energy background radiation

Page 3: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 3

Hard x-ray mirrors

Soft x-ray mirrors

~14m

X-ray mirror locations in FEE

Page 4: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 4

Page 5: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 5

Page 6: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 6

NEH

X-ray pump-probe

AMO SXR

soft x-ray line

hard x-ray line

Hutch 1 Hutch 2 Hutch 3

Page 7: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 7

FEH

XPCS Coherent x-ray

imaging

High energy density science

Hutch 4Hutch 5 Hutch 6

Page 8: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 8

Effects of Mirror Imperfections

Imperfections happen on all length scalesPower Spectral Density function (PSD) typically shows fractal power law behavior (with smaller errors at shorter wavelengths)

RoughnessErrors on x-ray wavelength scale

Cause scatter far out of direct beam

Slope errorsErrors on micron scale (larger than , but small compared to beam footprint)

Cause broadening of beam divergence

Page 9: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 9

100 80 60 40 20 0 20 40 60 80 100

1.10

5

1.10

4

1.10

3

0.01

0.1

1

Ideal FEL Beam

Offset Mirror Output

: 0.15 , 0.5 Scattering and Divergence Increase nm microradian errors

( )Vertical Angle to Beam Axis microradian

( )FEL Intensity normalized to ideal beam

Beam profile downstream of imperfect mirror

Ideal beam

Beam distorted by mirror

Broadening due to slope error

Scatter due to roughness

Page 10: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 10

For the LCLS, mirror roughness should not be a big problem. Realistic values of roughness will remove <5% of the beam intensity from the central spot.

Slope errors will broaden the beam and reduce its brightness. This is our major concern.

Page 11: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 11

We considered three cases for slope error:rms = 1 µrad, 0.5µrad, and 0.1µrad

1 µrad mirrors are readily available from several vendors

0.5 µrad mirrors are probably available, for a price

0.1 µrad mirrors may not be available today, but will be within a few years

The state of the art for 1m-length mirrors:

Page 12: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 12

Note: shorter mirrors are better

(World record: 0.01µrad rms, for a 100mm-long mirror)

The 1m length of the LCLS hard x-ray mirrors is driven by the desire to reflect 24keV radiation, and the desire to accept all of the beam at 2 keV, and still not hit the end regions of the mirror.

Also note: the soft x-ray mirrors are short. They operate at a steeper angle, so a length of only 100-200mm is needed.

Page 13: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 13

0.4 0.2 0 0.2 0.4

0.4

0.2

0

0.2

0.4

1 microradian error0.5 microradian error0.1 microradian error

NEH1 FWHM Contours for 1.5 nm

Horizontal Axis (mm)

Vertical Axis (mm)

NEH Hutch 1

1.0 µrad Slope Errors

0.5 µrad Slope Errors

0.1 µradSlope ErrorsHorizontal Axis

_max _min _max _min _max _min

Effective Source Distance (m) 102.6 75.4 118.8 105.3 126.4 134.0FWHM Source Divergence (µrad) 10.53 7.68 8.80 4.99 8.17 3.73FWHM Beam Size in Hutch (µm) 1083.3 584.4 1048.6 530.8 1035.9 505.7

800eV 2keV 2keV 2keV800eV 800eV

Using short B4C mirrors at 15mrad incidence

z=117.1m (distance from end of undulator)

Vertical Axis _max _min

Source Distance (m) 127.2 138.2FWHM Source Size (µm) 81.59 76.03FWHM Source Divergence (µrad) 8.11 3.60FWHM Beam Size in Hutch (µm) 1034.8 503.1

800eV 2keV

Page 14: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 14

0.6 0.4 0.2 0 0.2 0.4 0.6

0.6

0.4

0.2

0

0.2

0.4

0.6

1 microradian error0.5 microradian error0.1 microradian error

NEH2 FWHM Contours for 1.5 nm

Horizontal Axis (mm)

Vertical Axis (mm)

1.0 µrad Slope Errors

0.5 µrad Slope Errors

0.1 µradSlope ErrorsHorizontal Axis

_max _min _max _min _max _min

Effective Source Distance (m) 113.6 86.4 129.8 116.3 137.4 145.0FWHM Source Divergence (µrad) 10.53 7.68 8.80 4.99 8.17 3.73FWHM Beam Size in Hutch (µm) 1198.8 668.3 1145.1 585.1 1125.5 546.3

800eV 800eV 800eV2keV 2keV 2keV

NEH Hutch 2

Using short B4C mirrors at 15mrad incidence

z=128.1m

Vertical Axis _max _min

Source Distance (m) 138.2 149.2FWHM Source Size (µm) 81.59 76.03FWHM Source Divergence (µrad) 8.11 3.60FWHM Beam Size in Hutch (µm) 1123.8 542.3

800eV 2keV

Page 15: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 15

0.2 0.1 0 0.1 0.2

0.2

0.1

0

0.1

0.2

1 microradian error0.5 microradian error0.1 microradian error

NEH3 FWHM Contours for 0.15 nm

Horizontal Axis (mm)

Vertical Axis (mm)

1.0 µrad Slope Errors

0.5 µrad Slope Errors

0.1 µradSlope ErrorsVertical Axis

_min _max _min _max _min _max

Effective Source Distance (m) 62.9 95.7 86.3 127.4 170.0 157.8FWHM Source Divergence (µrad) 6.77 7.57 3.52 4.90 1.30 3.66FWHM Beam Size in Hutch (µm) 430.6 728.8 310.0 629.1 228.4 582.8

8keV 8keV 8keV2keV 2keV 2keV

NEH Hutch 3

Using 1m SiC mirrors at 1.3mrad incidence

z=138.8m

Horizontal Axis _min _max

Source Distance (m) 193.1 159.9FWHM Source Size (µm) 59.94 76.03FWHM Source Divergence (µrad) 1.10 3.60FWHM Beam Size in Hutch (µm) 221.4 580.4

8keV 2keV

Page 16: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 16

1 0.5 0 0.5 11

0.5

0

0.5

1

1 microradian error0.5 microradian error0.1 microradian error

FEH1 FWHM Contours for 0.15 nm

Horizontal Axis (mm)

Vertical Axis (mm)

1.0 µrad Slope Errors

0.5 µrad Slope Errors

0.1 µradSlope ErrorsVertical Axis

_min _max _min _max _min _max

Effective Source Distance (m) 289.0 321.8 312.4 353.5 396.0 383.9FWHM Source Divergence (µrad) 6.77 7.57 3.52 4.90 1.30 3.66FWHM Beam Size in Hutch (µm) 1958.9 2438.1 1102.3 1735.0 517.2 1407.6

8keV 8keV 8keV2keV 2keV 2keV

FEH Hutch 4

Using 1m SiC mirrors at 1.3mrad incidence

z=364.9m

Horizontal Axis _min _max

Source Distance (m) 419.2 386.0FWHM Source Size (µm) 59.94 76.03FWHM Source Divergence (µrad) 1.10 3.60FWHM Beam Size in Hutch (µm) 466.6 1391.0

8keV 2keV

Page 17: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 17

1 0.5 0 0.5 1

1

0.5

0

0.5

1

1 microradian error0.5 microradian error0.1 microradian error

FEH2 FWHM Contours for 0.15 nm

Horizontal Axis (mm)

Vertical Axis (mm)

1.0 µrad Slope Errors

0.5 µrad Slope Errors

0.1 µradSlope ErrorsVertical Axis

_min _max _min _max _min _max

Effective Source Distance (m) 309.6 342.4 333.0 374.1 416.6 404.5FWHM Source Divergence (µrad) 6.77 7.57 3.52 4.90 1.30 3.66FWHM Beam Size in Hutch (µm) 2098.4 2594.0 1174.8 1835.9 543.7 1482.9

8keV 8keV 8keV2keV 2keV 2keV

FEH Hutch 5

Using 1m SiC mirrors at 1.3mrad incidence

z=385.5m

Horizontal Axis _min _max

Source Distance (m) 439.8 404.6FWHM Source Size (µm) 59.94 76.03FWHM Source Divergence (µrad) 1.10 3.60FWHM Beam Size in Hutch (µm) 489.2 1465.0

8keV 2keV

Page 18: John Arthur Mirror effectsjarthur@slac.stanford.edu June 23, 2006 1 Effects of LCLS X-Ray Mirrors John Arthur Presenting work by Peter Stefan and Mike

John Arthur

Mirror effects [email protected]

June 23, 2006 18

1 0.5 0 0.5 1

1

0.5

0

0.5

1

1 microradian error0.5 microradian error0.1 microradian error

FEH3 FWHM Contours for 0.15 nm

Horizontal Axis (mm)

Vertical Axis (mm)

1.0 µrad Slope Errors

0.5 µrad Slope Errors

0.1 µradSlope ErrorsVertical Axis

_min _max _min _max _min _max

Effective Source Distance (m) 330.2 363.0 353.6 394.7 437.3 425.1FWHM Source Divergence (µrad) 6.77 7.57 3.52 4.90 1.30 3.66FWHM Beam Size in Hutch (µm) 2237.9 2749.9 1247.3 1936.9 570.3 1558.2

8keV 8keV 8keV2keV 2keV 2keV

FEH Hutch 6

Using 1m SiC mirrors at 1.3mrad incidence

z= 406.1m

Horizontal Axis _min _max

Source Distance (m) 460.4 427.2FWHM Source Size (µm) 59.94 76.03FWHM Source Divergence (µrad) 1.10 3.60FWHM Beam Size in Hutch (µm) 511.8 1539.0

8keV 2keV