Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock

In this paper, we present a model characterizing the interaction of a radiative shock (RS) with a solid material, as described in a recent paper (Koenig et al., Phys. Plasmas, 24, 082707 (2017)), the new model is then related to recent experiments performed on the GEKKO XII laser facility. The RS ge...

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Հիմնական հեղինակներ: Michel, T, Falize, E, Albertazzi, B, Rigon, G, Sakawa, Y, Gregori, G, al., E
Ձևաչափ: Journal article
Հրապարակվել է: Cambridge University Press 2018
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author Michel, T
Falize, E
Albertazzi, B
Rigon, G
Sakawa, Y
Gregori, G
al., E
author_facet Michel, T
Falize, E
Albertazzi, B
Rigon, G
Sakawa, Y
Gregori, G
al., E
author_sort Michel, T
collection OXFORD
description In this paper, we present a model characterizing the interaction of a radiative shock (RS) with a solid material, as described in a recent paper (Koenig et al., Phys. Plasmas, 24, 082707 (2017)), the new model is then related to recent experiments performed on the GEKKO XII laser facility. The RS generated in a xenon gas cell propagates towards a solid obstacle that is ablated by radiation coming from the shock front and the radiative precursor, mimicking processes occurring in astrophysical phenomena. The model presented here calculates the dynamics of the obstacle expansion, which depends on several parameters, notably the geometry and the temperature of the shock. All parameters required for the model have been obtained from experiments. Good agreement between experimental data and the model is found when spherical geometry is taken into account. As a consequence, this model is a useful and easy tool to infer parameters from experimental data (such as the shock temperature), and also to design future experiments.
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spelling oxford-uuid:ce96d06c-0cee-401a-b74d-2d26dd5137572022-03-27T07:36:37ZAnalytical modelling of the expansion of a solid obstacle interacting with a radiative shockJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:ce96d06c-0cee-401a-b74d-2d26dd513757Symplectic Elements at OxfordCambridge University Press2018Michel, TFalize, EAlbertazzi, BRigon, GSakawa, YGregori, Gal., EIn this paper, we present a model characterizing the interaction of a radiative shock (RS) with a solid material, as described in a recent paper (Koenig et al., Phys. Plasmas, 24, 082707 (2017)), the new model is then related to recent experiments performed on the GEKKO XII laser facility. The RS generated in a xenon gas cell propagates towards a solid obstacle that is ablated by radiation coming from the shock front and the radiative precursor, mimicking processes occurring in astrophysical phenomena. The model presented here calculates the dynamics of the obstacle expansion, which depends on several parameters, notably the geometry and the temperature of the shock. All parameters required for the model have been obtained from experiments. Good agreement between experimental data and the model is found when spherical geometry is taken into account. As a consequence, this model is a useful and easy tool to infer parameters from experimental data (such as the shock temperature), and also to design future experiments.
spellingShingle Michel, T
Falize, E
Albertazzi, B
Rigon, G
Sakawa, Y
Gregori, G
al., E
Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
title Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
title_full Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
title_fullStr Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
title_full_unstemmed Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
title_short Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
title_sort analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
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