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Parameters of supersonic astrophysically-relevant plasma jets collimating via poloidal magnetic field measured by x-ray spectroscopy method

  • E. D. Filippov
  • , S. A. Pikuz
  • , I. Yu Skobelev
  • , S. N. Ryazantsev
  • , D. P. Higginson
  • , D. Khaghani
  • , G. Revet
  • , S. N. Chen
  • , J. Fuchs
  • Joint Institute for High Temperatures of the Russian Academy of Sciences
  • Lawrence Livermore National Laboratory
  • GSI Helmholtzzentrum fur Schwerionenforschung

Résultats de recherche: Contribution à un journalArticle de conférenceRevue par des pairs

Résumé

Application of external magnetic field to a laser-generated plasma flows allows to investigate stable, large aspect ratio plasma jets which are relevant to a number of astrophysical cases. In the experiment with 0.6 ns, 40 J laser pulses focused to 700 μm focal spot at solid CF2 target in presence of 20 T poloidal magnetic field the parameters of the plasma jet were studied by means of spatially resolved x-ray spectroscopy. Focusing spectrometer with spatial resolution was used to record the temporally-integrated x-ray emission spectra of the plasma with spatial resolution along the jet propagation. Using the relative intensities of spectral lines emitted by F He-like ions, the electron temperature Te and density Ne profiles of the plasma are obtained. It is shown that Ne decreases monotonically in the case without B-field, but demonstrates an extended density profile up to 10 mm when 20 T magnetic field is applied. Ne values are consistent with that observed via interferometry diagnostics, thus providing the confidence in our x-ray spectroscopy analysis techniques.

langue originaleAnglais
Numéro d'article012114
journalJournal of Physics: Conference Series
Volume774
Numéro de publication1
Les DOIs
étatPublié - 27 nov. 2016
Evénement31st International Conference on Equations of State for Matter, ELBRUS 2016 - Elbrus, Russie
Durée: 1 mars 20166 mars 2016

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