Dual-channel compressed ultrafast photography for Z-pinch dynamic imaging

The compressed ultrafast photography (CUP) can capture non-repetitive time-evolving events at 7 × 1013 fps, which is anticipated to find a diverse range of applications in physics, biomedical imaging, and materials science. The feasibility of diagnosing ultrafast phenomenon of Z-pinch by using the C...

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Veröffentlicht in:Review of scientific instruments 2023-03, Vol.94 (3), p.035106-035106
Hauptverfasser: Yao, Z. M., Sheng, L., Song, Y., Hei, D. W., Li, Y., Zhu, Z. J., Zhou, H. Y., Yan, W. P., Han, C. C., Duan, B. J., Yang, K. X., Peng, B. D., Zhang, S. A., Qi, D. L., Jin, C. Z., Yao, Y. H., Huang, Z. Q.
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Sprache:eng
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Zusammenfassung:The compressed ultrafast photography (CUP) can capture non-repetitive time-evolving events at 7 × 1013 fps, which is anticipated to find a diverse range of applications in physics, biomedical imaging, and materials science. The feasibility of diagnosing ultrafast phenomenon of Z-pinch by using the CUP has been analyzed in this article. Specifically, a dual-channel CUP design has been adopted for acquiring high quality reconstructed images and the strategies of identical masks, uncorrelated masks, and complementary masks have been compared. Furthermore, the image of the first channel was rotated by 90° to balance the spatial resolution between the sweep direction and the non-sweep direction. Both five synthetic videos and two simulated Z-pinch videos were chosen as the ground truth to validate this approach. The average peak signal to noise ratio of the reconstruction results is 50.55 dB for the self-emission visible light video and 32.53 dB for the laser shadowgraph video with unrelated masks (rotated channel 1). The simulation results show that the time–space-evolving process of plasma distribution can be well retold, and the phenomenon of plasma instability can be accurately diagnosed by the dual-channel CUP with unrelated masks (rotated channel 1). This study may promote the practical applications of the CUP in the field of accelerator physics.
ISSN:0034-6748
1089-7623
DOI:10.1063/5.0127056