Speckle contrast of interfering fluorescence X-rays.
X-ray fluorescence
XPCS
incoherent diffraction imaging
speckle contrast estimation
Journal
Journal of synchrotron radiation
ISSN: 1600-5775
Titre abrégé: J Synchrotron Radiat
Pays: United States
ID NLM: 9888878
Informations de publication
Date de publication:
01 Jan 2023
01 Jan 2023
Historique:
received:
09
03
2022
accepted:
12
10
2022
entrez:
5
1
2023
pubmed:
6
1
2023
medline:
6
1
2023
Statut:
ppublish
Résumé
With the development of X-ray free-electron lasers (XFELs), producing pulses of femtosecond durations comparable with the coherence times of X-ray fluorescence, it has become possible to observe intensity-intensity correlations due to the interference of emission from independent atoms. This has been used to compare durations of X-ray pulses and to measure the size of a focusedX-ray beam, for example. Here it is shown that it is also possible to observe the interference of fluorescence photons through the measurement of the speckle contrast of angle-resolved fluorescence patterns. Speckle contrast is often used as a measure of the degree of coherence of the incident beam or the fluctuations of the illuminated sample as determined from X-ray diffraction patterns formed by elastic scattering, rather than from fluorescence patterns as addressed here. Commonly used approaches to estimate speckle contrast were found to suffer when applied to XFEL-generated fluorescence patterns due to low photon counts and a significant variation of the excitation pulse energy from shot to shot. A new method to reliably estimate speckle contrast under such conditions, using a weighting scheme, is introduced. The method is demonstrated by comparing the speckle contrast of fluorescence observed with pulses of 3 fs to 15 fs duration.
Identifiants
pubmed: 36601922
pii: S1600577522009997
doi: 10.1107/S1600577522009997
pmc: PMC9814059
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM
Pagination
11-23Subventions
Organisme : Deutsche Forschungsgemeinschaft
ID : 390715994
Organisme : Helmholtz Association
ID : ExNet-0002
Organisme : Vetenskapsrådet
ID : Grant 2019-03935
Organisme : Vetenskapsrådet
ID : 2018-00740
Informations de copyright
open access.
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