Hostname: page-component-76d6cb85b7-92wsb Total loading time: 0 Render date: 2026-07-11T11:48:04.114Z Has data issue: false hasContentIssue false

A novel multi-shot target platform for laser-driven laboratory astrophysics experiments

Published online by Cambridge University Press:  09 February 2023

Pablo Perez-Martin*
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany Technische Universität Dresden, Dresden, Germany
Irene Prencipe
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany
Manfred Sobiella
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany
Fabian Donat
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany
Ning Kang
Affiliation:
Key Laboratory of High Power Laser and Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai, China
Zhiyu He
Affiliation:
Shanghai Institute of Laser Plasma, China Academy of Engineering Physics, Shanghai, China
Huiya Liu
Affiliation:
Key Laboratory of High Power Laser and Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai, China
Lei Ren
Affiliation:
Key Laboratory of High Power Laser and Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai, China
Zhiyong Xie
Affiliation:
Shanghai Institute of Laser Plasma, China Academy of Engineering Physics, Shanghai, China
Jun Xiong
Affiliation:
Shanghai Institute of Laser Plasma, China Academy of Engineering Physics, Shanghai, China
Yan Zhang
Affiliation:
Key Laboratory of High Power Laser and Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai, China
Florian-Emanuel Brack
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany Technische Universität Dresden, Dresden, Germany
Michal Červenák
Affiliation:
Institute of Plasma Physics, Czech Academy of Sciences, Prague, Czech Republic
Pavel Gajdoš
Affiliation:
Institute of Plasma Physics, Czech Academy of Sciences, Prague, Czech Republic Czech Technical University, Faculty of Nuclear Sciences and Physical Engineering, Prague, Czech Republic
Lenka Hronová
Affiliation:
Institute of Plasma Physics, Czech Academy of Sciences, Prague, Czech Republic Czech Technical University, Faculty of Nuclear Sciences and Physical Engineering, Prague, Czech Republic
Kakolee Kaniz
Affiliation:
Department of Physics, Jagannath University, Dhaka, Bangladesh
Michaela Kozlová
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany Institute of Plasma Physics, Czech Academy of Sciences, Prague, Czech Republic ELI-Beamlines, Institute of Physics, Czech Academy of Sciences, Prague, Czech Republic
Florian Kroll
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany
Xiayun Pan
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany Technische Universität Dresden, Dresden, Germany
Gabriel Schaumann
Affiliation:
Institute for Nuclear Physics, Technical University of Darmstadt, Darmstadt, Germany
Sushil Singh
Affiliation:
Institute of Plasma Physics, Czech Academy of Sciences, Prague, Czech Republic Institute of Physics, Czech Academy of Sciences, Prague, Czech Republic
Michal Šmíd
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany
Francisco Suzuki-Vidal
Affiliation:
Blackett Laboratory, Imperial College, London, United Kingdom First Light Fusion, Oxford Industrial Park, Yarnton, Oxford, United Kingdom
Panzheng Zhang
Affiliation:
Key Laboratory of High Power Laser and Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai, China
Jinren Sun
Affiliation:
Shanghai Institute of Laser Plasma, China Academy of Engineering Physics, Shanghai, China
Jianqiang Zhu
Affiliation:
Key Laboratory of High Power Laser and Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai, China
Miroslav Krůs
Affiliation:
Institute of Plasma Physics, Czech Academy of Sciences, Prague, Czech Republic
Katerina Falk
Affiliation:
Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, Germany Technische Universität Dresden, Dresden, Germany Institute of Physics, Czech Academy of Sciences, Prague, Czech Republic
*
Correspondence to: Pablo Perez-Martin, Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Bautzner Landstraße 400, 01328 Dresden, Germany. Email: p.perez-martin@hzdr.de

Abstract

A new approach to target development for laboratory astrophysics experiments at high-power laser facilities is presented. With the dawn of high-power lasers, laboratory astrophysics has emerged as a field, bringing insight into physical processes in astrophysical objects, such as the formation of stars. An important factor for success in these experiments is targetry. To date, targets have mainly relied on expensive and challenging microfabrication methods. The design presented incorporates replaceable machined parts that assemble into a structure that defines the experimental geometry. This can make targets cheaper and faster to manufacture, while maintaining robustness and reproducibility. The platform is intended for experiments on plasma flows, but it is flexible and may be adapted to the constraints of other experimental setups. Examples of targets used in experimental campaigns are shown, including a design for insertion in a high magnetic field coil. Experimental results are included, demonstrating the performance of the targets.

Information

Type
Research Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press in association with Chinese Laser Press
Figure 0

Figure 1 Schematic views of the target assembly: (a) side view of the laser–target interaction; (b) 3D visualization of a target assembly with laser cones.

Figure 1

Figure 2 Comparison between variant target assemblies for different experiments on astrophysical flows: (a) design for experiments on flow collisions with static objects; (b) design for experiments on collisions of counter-propagating flows, also depicted in Figure 1(b).

Figure 2

Figure 3 Representations of the microfabricated radiography backlighter: (a) schematic; (b) magnified view; (c) full view of the backlighter plate attached to a target assembly.

Figure 3

Figure 4 Components of a target assembly for use inside a magnetic coil.

Figure 4

Figure 5 3D representations of a target assembly inserted into a split pair coil: (a) side view; (b) cross-section. The basic interaction that is studied remains the same as shown in Figure 1(a), with the laser focusing on a thin foil sample and generating a plasma flow in the center of the coils.

Figure 5

Figure 6 Alignment bench used for alignment of a magnetic field target. The target assembly can be directly taken out of the bench and inserted into the coil, where it would sit at an already aligned position.

Figure 6

Figure 7 Schematic of the experimental setup for the SG-II campaign. Four beams come from each side, each carrying 250 J of energy, for a total of 1 kJ. The separation between samples is 3.6 mm, and the beams on each side are set to different delays depending on the samples being studied, to ensure the resulting flows meet roughly at the middle of the observation window. The backlighter depicted follows the design shown in Figure 3, and the timing of its driver laser is determined depending on the expected velocity of the plasma flows.

Figure 7

Figure 8 Target changes introduced to optimize the radiography diagnostic at SG-II. Both images show two colliding plasma flows, one formed from a 10 μm titanium foil, coming from the top, and one from a 6 μm polyethylene terephthalate (PET) foil, from the bottom. The latter cannot be seen in the radiography due to the low X-ray absorption of PET. The separation between the samples is 3.6 mm, but the initial 0.3 mm of propagation of each flow is blocked by the target body. In the initial case without shielding, the self-emission of the plasma plume that expands from the interaction area and that of trapped material inside gaps in the target body are able to reach the X-ray diagnostic, projecting a bright stripe into the radiography (a). By adding shielding and eliminating any of the gaps on the assembly, this emission can be blocked and the results are cleaner (b).

Figure 8

Figure 9 Streaked optical self-emission of a single flow from a 10 μm aluminum sample, obtained during the SG-II campaign. The flow velocity can be calculated by tracking the maximum of the detected self-emission over time, and then fitting those points to a line using the least squares method. The flow in the image traverses 900 μm in 12 ns, which corresponds to the velocity of 75 km/s.

Figure 9

Figure 10 Schematic of the experimental setup for the PALS campaign.

Figure 10

Figure 11 Interferometry results for a flow from a 6 um aluminum foil under the conditions detailed in Figure 10 (a) with the target design for unmagnetized flows (Figure 2(a)), and with the magnetic field target (Figure 5) inserted inside the coil with (b) no field, (c) a 5 T field and (d) a 10 T field. All images are taken using a Grasshopper3 U3-28S4 charge-coupled device integrated over 0.3 ns. The limited space and exhaust capacities inside the magnetic field targets cause an accumulation of material visible in the interferograms.