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HAL Id: jpa-00225870

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Submitted on 1 Jan 1986

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PARTIALLY COHERENT RADIATION AT X-RAY WAVELENGTHS

D. Attwood, K. Kim, N. Wang, N. Iskander

To cite this version:

D. Attwood, K. Kim, N. Wang, N. Iskander. PARTIALLY COHERENT RADIATION AT X-RAY WAVELENGTHS. Journal de Physique Colloques, 1986, 47 (C6), pp.C6-203-C6-210.

�10.1051/jphyscol:1986627�. �jpa-00225870�

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JOURNAL DE PHYSIQUE,

Colloque C6, suppl6ment au n o 10, Tome 47, octobre 1986

PARTIALLY COHERENT RADIATION AT X-RAY WAVELENGTHS

D. ATTWOOD, K.J. KIM, N. WANG and N. ISKANDER

C e n t e r f o r X - R a y Optics, L a w r e n c e B e r k e l e y L a b o r a t o r y , U n i v e r s i t y o f C a l i f o r n i a , B e r k e l e y , C A 94720, U. S. A.

Resume - Dans le document, nous discutons les attributs du rayonnement cohd- rent partiel produit par les lasers de produits par lasers. Nous discutons les propridtbs de coherence spatiale et temporelle, les expdriences li6es 1 la microscopie de rayons-X et 1 la microholographie qui profitent de de- gres varies de cohgrence. Nous illustrons, pour les valeurs de crste et de moyenne, le rendement radiatif en fonction de la puissance coh6rente et de

la luminositg spectrale.

Abstract - In this paper we discuss the properties of partially coherent radiation generated by X-ray lasers, undularcrrs, and laser produced plasmas.

We discuss spatial and temporal coherence properties, experiments involving X-ray microscopy and microholography which benefit from varying degrees of coherence, and we illustrate radi'ative performance in terms of both coherent power and spectral brightness, for both peak and average values.

Introduction

In recent years we have seen a significant advance in the ability to generate coherent radiation at ever shorter wavelengths - now extending throughout the ultraviolet and into the x-ray region of the electromagnetic spectrum. These are particularly interesting spectral regions for

applications in many scientific and technological disciplines. Because the wavelength is short, the radiation can be used to both "see" and "write"

patterns of small feature size. Thus one can form high spatial resolution x-ray microscopes and microprobes and can fabricate yet more powerful integrated circuits. The photon energy is particularly interesting as it coincides with the many atomic and molecular transition resonances which pervade this region of the spectrum. The new accessibility of this region, provided both high brightness sources and requisite x-ray optics are

available, will permit the utilization of many exciting techniques. Element specific bio-dynamics, site specific photochemical processing, polarization sensitive scattering studies of chiral structures, element specific studies of surface state formation, and dynamical studies of thin film and lattice structure formation are, to name a few, fields which would benefit from the unique capabilities of elemental sensitivity and high space-time resolution.

Coherence Requirements

An example of an experimental technique which would benefit many of the above cited sciences is that of an x-ray microprobe. As illustrated in figure 1, a Fresnel zone plate might be used to concentrate radiation in a small

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1986627

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C6-204 JOURNAL DE PHYSIQUE

focal spot area. The radiation could be used to probe, stimulate or scan any of a variety of chemically, physically or biologically interesting systems.

The size of the focal region is dependent upon both the spatial and temporal properties of the incident radiation. For spatially coherent radiation a focal spot diameter (waist) of 2.4Ar will be obtained with a zone plate of outer zone width Ar. Resolution, as defined by Rayleigh, would be 1.2Ar.

A zone plate of outer zone width of 500 A would give a focal spot diameter of approximately 1200 A. To achieve this diffraction limited focusing it is necessary that the zone plate be perfect to a fraction of a wavelength, and that the radiation emanate from an uncertainty limited phase space

characterized by 8-8 = A/2. If the radiation is characterized by a larger phase space, the resulting focal spot will be proportionally larger and the resolution proportionally degraded. The zone plate microprobe also requires a degree of temporal (longitudinal) coherence, albeit modest. In order to avoid blurring of the focal region by chromatic aberration, the radiation must possess a coherence length (distance over which interference effects are significant) Qc = A2/bA, at least as large as the coherence

requirements of the zone plate, blA/2, where bl is the number of Fresnel zones. Generally this is a modest requirement: with bl = 500 and A -- 30 A, one requires Qc A somewhat more demanding experiment is that of off-axis x-ray - lpm.

microholography, as illustrated in figure 2. In this case the ZP does not form an image in the recording plahe, but rather it gathers the high frequency (large angle) scattered radiation (containing details of the smaller sample features) and directs it back toward the recording medium where it is encoded through interference with a plane or spherical reference wave generated by the nearby diffraction grating. The scattered radiation is thus heterodyned by the reference wave, with a carrier spatial frequency roughly that of the grating, allowing use of a lower resolution but more sensitive recorder (perhaps x-ray film) than would otherwise be possible. Both spatial and temporal coherence requirements are more demanding in the holographic case, requiring spatially coherent illumination over a field wider by some factor, and a temporal coherence length increased by that factor squared, e.g. if the grating extends laterally to a distance of five ZP radii, then the temporal coherence must be increased by a factor of twenty-five. Thus one would require full spatial coherence and a longitudinal coherence of 20 pm.

Radiation Sources

The generation of partially coherent radiation, combined with requisite spatial and temporal filtering, can be achieved in several ways. Figures 3-5 illustrate an atomic laser, a magnetic undulator, and a laser-produced, hot-dense plasma emitting x-rays into 2s steradians. All three can generate radiation at XW wavelengths, and perhaps it can be said that all are

partially coherent - certainly all could be used as the source of radiation in figures 1 and 2. The differences are the degree of coherence, determining the amount of spatial and temporal filtering required for a particular

application; the average a?d peak power produced; and the shortness of the wavelength and its nearness to the atomic and molecular resonances of interest.

Radiative Performance

In figures 6-8 we show generated coherent power and spectral brightness, for both average and peak values, and for a variety of spectral widths (coherence lengths). In the estimates of coherent power, only that portion of the radiation within d-8 = A/2 is accepted, such that full spatial coherence would result. In addition, perfect optics are assumed - no aberrations, 100%

efficiency. The need for several illustrations is due to the wide variety of

applications one can envision, some requiring minimal coherence, others

requiring substantial coherence. Upon inspection one readily sees that each

of the radiation sources has its own advantages.

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References

1. D.L. Hatthews et al., Phys. Rev. Letters, 54, 110, 1985; M.D. Rosen et al., Phys Rev. Letters, 54, 106, 1985.

2. D.T. Attwood, K-J. Kim, K. Halbach, and H.R. Howells, "Undulators as a Primary Source of Coherent X-rays", paper presented at the International Conference on Insertion Devices for Synchrotron Sources, October 1985;

also published as Lawrence Berkeley Laboratory PUB-20569, 1985.

3. Recent (June, 1986) undulator experiments are reported by H. Rarbaek, Brookhaven National Laboratory, Upton. New York.

4. D.W. Phillion, E.H. Campbell et al.. to be published; D.T. Attwood, N.M. Ceglio, E.H. Campbell, J.T. Larson, D.H. Hatthews, and S.L. Lane,

"Compression Heasurements in Laser-Driven Implosion Experiments", Laser

Interaction and Related Plasma Phenomenon, (Plenum, New York, 1981) eds.

H.J. Schwarz. H. Hora, M.J. Lubin, and B. Yaakobi; B. Yaakobi et al., Optics Communications, 33, 196, 1981.

5. Nasif Iskander and Nadine Wang, Optical Society of America, Topical Conference on Short Wavelength Coherent Radiation. Honterey. CA, April 1986.

zones

Resolution = 1.2 FA = 1.2 Ar D = 4NAr

Figure 1. An x-ray microprobe based on use of a Presnel zone plate.

Spatially coherent radiation is focused to the smallest possible focal spot, of diameter 2.4Ar. Longitudinal (temporal)

coherence equal to N W 2 is required to avoid chromatic

defocusing effects, where N is the number of zones. Thus both

temporal and spatial coherence are required.

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JOURNAL DE PHYSIQUE

lograrn

coherent x-rays

Figure 2. Three dimensional imaging using OFF-axis holography.

As

in figure 1, full spatial coherence is required. Temporal coherence requirements increase as the square of the zone plate/diFFraction grating aperture.

Laser Radiation and Partial Coherence

Best Spatial and Temporal Coherence Longitudinal Transverse mode selector mode selector

b--.

Gain medium . T E M ~ ~ .

+ flash lamp -- 10-6

X

Poor Spatial, Less Temporal Coherence

6- - More power. less phase

---

-

L

correlation Gain medium

+ flash lamp

Figure 3. Two forms of lasers are illustrated. The First utilizes cavity mirrors, and internal mode selecting (filtering). The second is a high gain, single pass laser, employing no internal filtering.

and thus producing radiation of lesser coherence properties.

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Magnetlc undulator

r

(N periods)

Relat~vtstlc electron A

- L

beam - 2-r2

lux-concentrat~ng steel (Fe) pole Pieces I ' \i Permanent magnets

(SmCo5)

Figure 4. Undulator radiation produced by a relativistic electron beam traversing a periodic magnet structure. The radiation is partially coherent in nature. Spatial coherence is set by the phase space OF the electron beam and the wavelength.

Longitudinal coherence is set by the number of undulator periods.

Figure-5.- Narrow line emission from laser produced plasmas can provide

intense radiation at multi-keV photon energies, with competitive

coherence lengths. but require significant spatial filtering

(e.g. has no natural spatial coherence).

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C6-208 JOURNAL DE PHYSIQUE

( 6 4 Average Spectral Brightness in 0.1 % Bandwidth 1240.8, 1 2 4 A 1 2 A 1.2 A

C N O P C a

Photon Energy lev]

L

1 0 ' ~ ~ 100 l k 10k 100k

Pholon Energy lev]

(6-C) Peak Spectral Brightness in 0.01% Bandwidth 1

dZ

1240 A, 124 A 12 A 1 . 2 A

Peak Spectral Brightness in 0.1% Bandwidth

ldl

j

6 GeV I ESRF

I

I I 1 1 1 1 1 I I t 1

t

C N O P C a

I

I 6 GeV I ESRF

-

I

I

\

-

1 ' 1 'ALS Uo ALS U, \

'

I

-

1 -.;...t;.

1 1,.

.:.. ':I

1 0 ' ~ ~

1 0 100 l k 10k l00k

Photon Energy [eV]

Id0 -

ALS U,

,'--

8 '

\\

/,I/'

: . . . . .

I I

-

/ I : :

1 0 ' ~

-

10l8

-

TI Plasma

-

Figure 6. Average and peak values of spectral brightness in 0.1% and 0.01% bandwidths are plotted

f o r

the sources discussed here.

-

Existing Swrces

---

Proposed Sources

. . . . . . . . .

Harmonics

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(7-A)

Average Coherent Power in 1 pm Coherence Length

(7-8)

Peak Coherent Power in 1

pm Coherence Length

Photon Energy lev]

12408 1248. 128. 1.28.

A L s u v ~ ~ .

-,Uc

I drlrb' Ad8

I

ALS uA'\,

\>

\ \

$.

-

\

'!

I :\,;\\ ALS UD

p\

\\\\

\ \

I

',,ALS U, -

I I \

I 11,

I

10.'

\

10 I ,100 I #lk I 0 10k lOOk

I

Photon Energy [eV]

Figure 7. Average and peak coherent power in a 1

prn

coherence length are

plotted for the sources discussed here.

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JOURNAL DE PHYSIQUE

(a -

A)

Peak Coherent Power in

1 0 0

pm Coherence Length

ALS U, I I

.

\ I

ALs

U\,\, ,

':\I \~,ALS u,

\\ I\+

\I \'

/,

\::\ALs U,

s 2 k e r q \

\\

(206 A)

'*

\: ALS US

I

: I

1 0 - ~ \\ \

NSLS

I I I I

10 100 l k 10k look

Photon Energy [eV]

Peak Coherent Power in

1 0 pm

Coherence Length

1240A 1 2 4 8 12.8 1 . 2 a 1 0' I I 1 1 ' 1 1 1 1 ' 1

C N O P C a

ALS-U, I

I \

W L

I ':\

ALS Us

~e ~ a s e r

I \

10-7; 10 I ,100 I ' $ l k 1 1ok 1mk

Photon Energy

[eV]

Figure 8 . Peak coherent power i n 10

p

and 100

pm

coherence lengths is

p l o t t e d f o r the sources discussed here.

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