The new beamline ALOISA, now operational at the Elettra Synchrotron, is designed for surface studies by means of several experimental techniques: surface x-ray diffraction and reflectivity, photoemission spectroscopy, photoelectron diffraction, e--Auger coincidence spectroscopy. A new monochromator has been specifically designed and realized for this multipurpose beamline: it makes use of a channel-cut Si crystal dispersive element for the 3-8 keV range and of a plane mirror-plane grating element for the 200-2000 eV range. Both dispersive elements share the same optical system. In the low energy range (200-900 eV) the spectral resolving power exceeds 5000 while maintaining a throughput higher than 1010photons/s/200mA/0.02%BW. In the case of the N2 1s → π* and Ne 1s → 3p transitions, the extremely high signal-to-noise ratio of the absorption spectra allowed a very accurate determination of the corresponding natural linewidth (116 ± 2 and 250 ± 10eV, respectively). Moreover, the vibrational structure of the CO-oxygen 1s → π* transition has been fully resolved. In the high energy range, the measured flux exceeds 1010photons/s/200 mA up to 6.5 keV with a resolving power of ∼7500. © 1999 American Institute of Physics.

Performance of the grating-crystal monochromator of the ALOISA beamline at the Elettra Synchrotron

NALETTO, GIAMPIERO;TONDELLO, GIUSEPPE
1999

Abstract

The new beamline ALOISA, now operational at the Elettra Synchrotron, is designed for surface studies by means of several experimental techniques: surface x-ray diffraction and reflectivity, photoemission spectroscopy, photoelectron diffraction, e--Auger coincidence spectroscopy. A new monochromator has been specifically designed and realized for this multipurpose beamline: it makes use of a channel-cut Si crystal dispersive element for the 3-8 keV range and of a plane mirror-plane grating element for the 200-2000 eV range. Both dispersive elements share the same optical system. In the low energy range (200-900 eV) the spectral resolving power exceeds 5000 while maintaining a throughput higher than 1010photons/s/200mA/0.02%BW. In the case of the N2 1s → π* and Ne 1s → 3p transitions, the extremely high signal-to-noise ratio of the absorption spectra allowed a very accurate determination of the corresponding natural linewidth (116 ± 2 and 250 ± 10eV, respectively). Moreover, the vibrational structure of the CO-oxygen 1s → π* transition has been fully resolved. In the high energy range, the measured flux exceeds 1010photons/s/200 mA up to 6.5 keV with a resolving power of ∼7500. © 1999 American Institute of Physics.
1999
File in questo prodotto:
Non ci sono file associati a questo prodotto.
Pubblicazioni consigliate

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/2465458
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 190
  • ???jsp.display-item.citation.isi??? 185
  • OpenAlex 185
social impact