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Propagation of laser-generated plasma jet in an ambient medium

  • B. Loupias
  • , E. Falize
  • , C. D. Gregory
  • , T. Vinci
  • , S. Pikuz
  • , J. Waugh
  • , M. Koenig
  • , A. Ravasio
  • , W. Nazarov
  • , C. Michaut
  • , S. Bouquet
  • , Y. Kuramitsu
  • , D. Seiichi
  • , N. C. Woolsey
  • , Y. Sakawa
  • , H. Takabe
  • , A. Schiavi
  • , S. Atzeni
  • CEA/UVSQ/CNRS
  • Joint Institute for High Temperatures of the Russian Academy of Sciences
  • University of York
  • University of St Andrews
  • LUTH - Laboratoire de l'Univers et de ses Theories
  • Osaka University
  • University of Rome

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

In this work we present experimental research related to laboratory astrophysics using an intense laser. The goal of these experiments is to investigate some of the complex features of young stellar objects and astrophysical outflows, in particular the plasma jet interaction with the interstellar medium. The relevance of these experiments to astrophysics is measured through similarity criteria (scaling laws). These ensure the similarity between the astrophysical object and the laboratory provided that the dimensionless numbers are equivalent. Consequently, measurements of the plasma parameters are crucial to link laboratory research to astrophysics as they are needed for the determination of these dimensionless numbers. In this context, we designed experiments to generate plasma jets using an intense laser, and to study the evolution in vacuum and in an ambient medium.

langue originaleAnglais
Numéro d'article124027
journalPlasma Physics and Controlled Fusion
Volume51
Numéro de publication12
Les DOIs
étatPublié - 24 nov. 2009

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