2022
DOI: 10.3390/sym14122536
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X-ray Self-Emission Imaging of Hydrodynamic Laser-Induced Astrophysical Phenomena

Abstract: In this article, we present an overview of the application of X-ray self-emission methods for the imaging of hydrodynamic astrophysical phenomena in laboratory-scale experiments. Typical diagnostic approaches, their advantages, drawbacks, and application perspectives are considered. We show that X-ray imaging and spectroscopy methods with 2D and even 1D spatial resolution are valuable for numerous laboratory astrophysical problems. Furthermore, the methods revealed the hydrodynamic evolution, the spatial shape… Show more

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Cited by 2 publications
(1 citation statement)
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“…As can be seen from the X-ray imaging model of single-component materials, the main factors affecting imaging are the source characteristics, the absorption coefficient of the detected element, and the thickness of the material. For high absorption ratio materials containing elemental 𝑀 𝑎 and elemental 𝑀 𝑏 , the element type is known, and imaging using the same ray source can be optimized using previous models [29][30][31]. The imaging process for materials with high absorption ratios is shown in Figure 2.…”
Section: Model Buildingmentioning
confidence: 99%
“…As can be seen from the X-ray imaging model of single-component materials, the main factors affecting imaging are the source characteristics, the absorption coefficient of the detected element, and the thickness of the material. For high absorption ratio materials containing elemental 𝑀 𝑎 and elemental 𝑀 𝑏 , the element type is known, and imaging using the same ray source can be optimized using previous models [29][30][31]. The imaging process for materials with high absorption ratios is shown in Figure 2.…”
Section: Model Buildingmentioning
confidence: 99%