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CheironSchool_Oct2010_Lec2.ppt 1 EUV and Soft X-Ray Beamlines Cheiron School October 2010 SPring-8 David Attwood University of California, Berkeley and Advanced Light Source, LBNL

EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Page 1: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 1

EUV and Soft X-Ray Beamlines

Cheiron School October 2010 SPring-8

David Attwood University of California, Berkeley

and Advanced Light Source, LBNL

Page 2: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Beamlines are used to transport photons to the sample, and take a desired spectral slice

2

Page 3: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

A typical beamline: monochromator plus focusing optics to deliver radiation to the sample

3

Page 4: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Typical parameters for synchrotron radiation

4

Page 5: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Undulator radiated power in the central cone

5

Page 6: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Power in the central radiation cone for three x-ray undulators

6

Page 7: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Typical parameters for synchrotron radiation

7

Page 8: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Time structure of synchrotron radiation

8

Page 9: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

High spectral resolution (meV beamline)

9 Courtesy of Zahid Hussein (ALS)

Page 10: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

Beamline 7.0 at Berkeley’s Advanced Light Source

10

Page 11: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

MAESTRO: A new varied-line-space grating monochromator beam line for angle-resolved-photo-electron-spectroscopy with high spectral and spatial resolution at the Advanced Light Source

11

Jason Wells, Derek Yegian, Ken Chow, Eli Rotenberg, Aaron Bostwick, Geoff Gaines and Tony Warwick

The latest soft x-ray undulator spectroscopy beam line planned for the ALS serves MAESTRO a new high resolution Angle Resolved Photo Emission facility with zone-plate focused nano-ARPES. The beam line design offers spectral resolution 1:30000 from 60eV to 400eV with an extended energy range from 20eV to 1000eV. Challenges include optical figure quality, thermal engineering, source size and stability and vibrations in the monochromator. The optical design is radical in that a VLS grating will provide all of the focusing in the dispersion direction, and the mirrors are plane, except for a sphere to collect and focus horizontally.

Courtesy of Eli Rotenberg and Tony Warwick (ALS)

Page 12: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

Varied line space gratings

12

1)  to erect the focal plane on a stationary set of exit slits

2)  to keep the zero-order light in focus, for easy tuning, and for monitoring of the photon energy.

Linear and non-linear line density variation

AFM measured groove shapes

The PEEM3 beam line at 11.0.2 uses a Triple-Ruled Varied-Line-Space grating:

Varied-Line-Space Plane Gratings provide focusing and aberration correction along with the dispersion that they generate in the monochromator. They can be used to erect the monochromator focal plane, making the position of the focus at the exit slit (almost) stationary as the grating rotates to select the photon energy. Beyond that, they are now being used to replace the focusing from shaped optics, making beam lines cheaper and easier to align.

Courtesy of Tony Warwick (ALS)

Page 13: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

MAESTRO: A new varied-line-space grating monochromator beam line at the ALS

13

9.25m

7.25m (to grating)

2.00m 0.80m 2.50m

~2.75m

0.50m

Maestro EPU

M202 G201a G201b G202a G202b

M211 M221

M212 M213 M214

Exit slit

Exit slit microARPES

nanoARPES Zone plate

Shield wall

Monochromator

Switch- yard

KB focusing mirrors

M201

Courtesy of Tony Warwick (ALS)

Page 14: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

MAESTRO at the ALS: gratings and efficiencies

14 Courtesy of Tony Warwick (ALS)

Page 15: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

Water-cooled optics are essential: correcting slope errors due to a thermal bump

15

Body plate showing pockets for cooling channels

Height error

Tangential slope error

Sagittal slope error

Courtesy of Tony Warwick (ALS)

Page 16: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

Ray tracing beamlines is an important tool

16

600lines_60eV_10000_c=4.02_18.7_0.038_1.5mmheatbumpcorrected

600lines_60eV_10000_c=3.93034_18.7_0.038_1.5mmheatbump

Significant degradation of the spectral resolution occurs due to localized heating of M202. It is almost entirely corrected by adjusting the monochromator focusing parameter from 3.93 to 4.02. The engineering design will allow this mirror to be built with 1mm thick hot-wall and the actual thermal deformation is expected to be less.

Courtesy of Tony Warwick (ALS)

Page 17: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

References

1

Reininger, R., Kriesel, K., Hulbert, S.L., Sanchez-Hanke, C. and Arena, D.A., Rev. Sci. Instrum.,79, 033108 2008

Peterson, H., Jung, C., Hellwig, C. Peatman, W.B. and Gudat, W., Rev. Sci. Instrum. 66 (1995) 1

Follath, R., and Senf, F., Nucl.Intrum. Methods Phys. Res. A390 (1997) 388

Amemiya, K., Kitajima, Y.,Ohta, T., and Ito, K., J. Synchrotron Radiation 3 (1996) 282

The original SHADOW package is available at www.nanotech.wisc.edu/CNTLABS/shadow.html and with an IDL user interface at www.esrf.fr/computing/scientific/xop

Undulator Radiation, Ellaume, P., in Undulators, Wigglers and their Applications,

Onuki, H. and Ellaume, P. eds., Taylor and Francis.

Characteristics of Synchrotron Radiation, Kim, K., J., in Xray Data Booklet LBNL internal report (1986) PUB 490 xdb.lbl.gov/xdb.pdf

D Fluckiger - Grating Solver Development Company Dec 2006 www.gsolver.com

Courtesy of Tony Warwick (ALS)

Page 18: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 2

Beamlines for spatially coherent undulator radiation

λ = 11.2 nm λ = 13.4 nm

1 µmD pinhole

25 mm wide CCD at 410 mm

Courtesy of Patrick Naulleau, LBNL.

Page 19: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherence at short wavelengths

3

Page 20: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Young’s double slit experiment: spatial coherence and the persistence of fringes

4

Page 21: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt

Spatial and spectral filtering to produce coherent radiation

5

Page 22: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Spatial and temporal coherence

6

Page 23: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Spatially filtered undulator radiation

Page 24: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Spatial and spectral filtering of undulator radiation

Page 25: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 9

Spatially and spectrally filtered undulator radiation

Page 26: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherent soft x-ray beamline: use of a higher harmonic (n = 3) to access shorter wavelengths

Page 27: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 11

Coherent soft x-ray science beamline

Rosfjord (UCB PhD thesis, 2004)

Energy range 200-1000eV Coherent flux at 600 eV: 2 × 1011 ph/sec/0.1%BW λ = 2.07 nm (600 eV)

• Wavefront interferomery to measure aberrations in zone plate lenses

• Measure material properties (f1 & f2)

• Develop new coherent soft x-ray optical techniques (Fourier Optics)

• Coherent scattering from magnetic nanostructures

K. Rosfjord, Y. Liu, D. Attwood, “Tunable Coherent Soft X-Rays”, IEEE J. Sel. Top. Quant. Electr.10, 1405 (Nov/Dec 2004)

Page 28: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Undulator beamline for high spatial coherence measurements

Page 29: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 13

Spatial coherence measurements of undulator radiation using the classic 2-pinhole technique

λ = 13.4 nm, 450 nm diameter pinholes, 1024 x 1024 EUV/CCD at 26 cm ALS, 1.9 GeV, λu = 8 cm, N = 55

Courtesy of Chang Chang, UC Berkeley and LBNL.

Page 30: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 14

Spatial coherence measurements of undulator radiation using the classic 2-pinhole technique

Courtesy of Chang Chang, UC Berkeley and LBNL.

λ = 13.4 nm, 450 nm diameter pinholes, 1024 x 1024 EUV/CCD at 26 cm ALS, 1.9 GeV, λu = 8 cm, N = 55

Page 31: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Spatial coherence measurements in the vertical plane

Courtesy of Chang Chang, UC Berkeley and LBNL.

λ = 13.4 nm, 450 nm diameter pinholes, 1024 x 1024 EUV/CCD at 26 cm ALS, 1.9 GeV, λu = 8 cm, N = 55

Page 32: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherent power for an EPU at the ALS

Page 33: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherent power at the Australian Synchrotron

Page 34: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherent power at SPring-8

Page 35: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherent soft x-ray beamline: use of a higher harmonic (n = 3) to access shorter wavelengths

Page 36: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 1

Coherent soft x-ray beamline: use of a higher harmonic (n = 3) to access shorter wavelengths

Page 37: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 2

Coherent Soft X-Ray Magnetic Scattering Endstation

Scattering in

Transmission

X rays

Sample location

Flangosaurus

Courtesy of K.Chesnel, S. Kevan, U. Oregon

Page 38: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 3

Example of experiment in transmission: coherent scattering from nanoparticles

Co Nanoparticles assembly precipitated on TEM grid

X-ray beam tuned to Co L3 resonant edge

Diffuse scattering

Pinhole (coherence)

CCD Camera 2048 x 2048

200 400 600 800 1000 1200 1400 1600 1800 2000

200

400

600

800

1000

1200

1400

1600

1800

2000

0.5

1

1.5

2

2.5

3

3.5

4

4.5

5

x 10 4

Scattering ring related to

interparticle distance ~12 nm

Courtesy of K.Chesnel, S. Kevan, U. Oregon

Page 39: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec2.ppt 4

Page 40: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Coherent power at BESSY II

Page 41: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Lensless imaging of magnetic nanostructures by x-ray spectro-holography

Page 42: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Undulators, FELs and coherence

Page 43: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Young’s double slit experiment: spatial coherence and the persistence of fringes

Page 44: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Young’s double slit experiment: spatial coherence and the persistence of fringes

Page 45: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Young’s double slit experiment with random emitters: Young did not have a laser

Page 46: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Young’s double slit experiment with phase coherent emitters (some lasers, or properly seeded FELs)

Page 47: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Undulators and FELs

Page 48: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Undulators and FELs

Page 49: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Undulators and FELs

“SASE” FEL – no seed (several separate “waves” �of electrons possible with uncorrelated phase.) �Less peak power, broader spectrum.

Page 50: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Seeded FEL

Second generation x-ray FELs.

Page 51: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Gain and saturation in an FEL

Page 52: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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Free Electron Lasers

Page 53: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

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References

18

Page 54: EUV and Soft X-Ray Beamlines - Cheiron School 2010cheiron2010.spring8.or.jp/text/lec/11_EUV.SX.BL_D.Attwood.pdf · harmonic (n = 3) to access shorter wavelengths . CheironSchool_Oct2010_Lec2.ppt

CheironSchool_Oct2010_Lec1.ppt

Lectures online at www.youtube.com

Amazon.com

19

UC Berkeley www.coe.berkeley.edu/AST/sxreuv www.coe.berkeley.edu/AST/srms

www.coe.berkeley.edu/AST/sxr2009