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Characterization of laser-driven Radiative shock of Astrophysical interests

Published online by Cambridge University Press:  18 July 2017

U. Chaulagain ,
C. Stehlé ,
J. Larour ,
M. Kozlová ,
F. Suzuki-Vidal ,
J. Nejdl  and
R. L. Singh
U. Chaulagain
Affiliation:
LERMA, Observatoire de Paris, UPMC, CNRS, 5 Pl. Janssen, 92195 Meudon, France
C. Stehlé
Affiliation:
LERMA, Observatoire de Paris, UPMC, CNRS, 5 Pl. Janssen, 92195 Meudon, France
J. Larour
Affiliation:
LPP, Ecole Polytechnique, UPMC, CNRS, 91128 Palaiseau, France
M. Kozlová
Affiliation:
Institute of Physics of ASCR, Na Slovance 2, 182 21 Prague 8, Czech Republic
F. Suzuki-Vidal
Affiliation:
The Blackett Laboratory, Imperial College, Prince Consort Road, London SW7 2AZ, UK
J. Nejdl
Affiliation:
Institute of Physics of ASCR, Na Slovance 2, 182 21 Prague 8, Czech Republic
R. L. Singh
Affiliation:
LERMA, Observatoire de Paris, UPMC, CNRS, 5 Pl. Janssen, 92195 Meudon, France LPP, Ecole Polytechnique, UPMC, CNRS, 91128 Palaiseau, France
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Abstract

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We highlight the recent experimental results on laser-driven radiative shock waves of astrophysical interests using kJ PALS laser facility. The generated shock is probed instantaneously by X-ray laser (λ = 21.2 nm) showing an unambiguous shock structure that includes both the post-shock and the precursor.

Keywords

Radiative shockX-ray laserstellar accretionlaboratory astrophysicsplasma
Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E28
Copyright
Copyright © International Astronomical Union 2017 

References

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