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Radiative heating of B, Al and Ni thin foils at 15-25 eV temperatures

  • C. Chenais-Popovics
  • , F. Gilleron
  • , M. Fajardo
  • , H. Merdji
  • , T. Mißalla
  • , J. C. Gauthier
  • , P. Renaudin
  • , S. Gary
  • , J. Bruneau
  • , F. Perrot
  • , T. Blenski
  • , W. Fölsner
  • , K. Eidmann
  • CEA/UVSQ/CNRS
  • Centre d'Etudes de Limeil-Valenton
  • DSM/SPAM
  • Max-Planck Institut für Quantenoptik

Research output: Contribution to journalArticlepeer-review

39 Citations (Scopus)

Abstract

Several thin foils have been heated by X-ray radiation emitted by a small gold cavity irradiated with the LULI facility Nd glass laser. The foils were heated to moderate temperatures (10-25 eV) in conditions near local thermodynamic equilibrium. Measurements of the absorption of Kα transitions of aluminum, of the K-shell transitions of boron, and of the n=2-3 and 4 transitions of nickel are reported. A 5000 l/mm transmission grating spectrograph recorded the boron data, and a flat thallium hydrogen phthalate (TlAP) crystal was used for aluminum and nickel absorption measurements. The nickel and aluminum spectra indicate a higher temperature (22-25 eV) than the boron case (14 eV), explained by a difference in the absorption spectra of these elements. In the Ni case the measured 2p-3d spin-orbit-split absorption structures compared well with theoretical spectra obtained with the SCO superconfiguration code using the spin orbit split transition arrays formalism (SOSA). The heating of the foils as calculated with radiative hydrodynamic simulations is very similar to the experimental data.

Original languageEnglish
Pages (from-to)117-133
Number of pages17
JournalJournal of Quantitative Spectroscopy and Radiative Transfer
Volume65
Issue number1-3
DOIs
Publication statusPublished - 7 Jan 2000
Externally publishedYes

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