Jul 2 – 6, 2018
Žofín Palace
Europe/Prague timezone

P5.2028 Multi-keV X-ray source generation at the Shenguang-III prototype

Jul 6, 2018, 2:00 PM
2h
Mánes

Mánes

Speaker

Gang Xiong

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P5.2028.pdf Multi-keV X-ray source generation at the Shenguang-III prototype Gang Xiong, Yunsong Dong, Yang Zhao, Bo Qing, Zhimin Hu, Minxi Wei, Tianming Song, Min Lv, Zhiyu Zhang, Guohong Yang, Jiyan Zhang, Jiamin Yang, Shaoen Jiang Research Center of Laser Fusion, China Academy of Engineering Physics, P. O. Box 919-986, Mianyang 621900, China Efficient multi-keV sources are essential in inertial confinement fusion and high energy density physics for radiography, opacity measurements, material testing, and so on[1-5]. In this talk, we present the recent progress in multi-keV sources developments at the Shenguang-III prototype laser facility. An underdense plasma mechanism was used to improve the laser-to-X-ray conversion efficiency. Main targets are small cylindrical cavities with 700-800 μm diameter, and 500-800 μm height. The main wall materials are Ti, V and Ni enclosed by CH tubes of 30 μm thick. Eight 3ω laser beams with total energy of about 6.4 kJ in a 1 ns square pulse were focused on the inner wall of the cavity. The absolute X-ray fluxes were measured by absolutely calibrated HXRDs and FXRDs for X-ray energy higher and lower than 4keV, respectively. HXRDs and FXRDs were installed at different angles for X-ray angular distribution measurements. K-shell X-ray spectra were recorded by crystal spectrometers. The electron temperatures were deduced from both the laser Thomson scatters and X-ray spectra. The time behaviors of the X-ray images in two energy ranges were recorded through an X-ray framing camera. The X-ray conversion efficiency was about 2-3 times higher than the traditional thick solid. Reference: [1] S. Tu et al., Phys. Plasmas 23, 013102 (2016). [2] Y. Dong et al., J. Appl. Phys. 115, 43305 (2014). [3] W. Shang et al., Appl. Phys. Lett. 102, 94105 (2013). [4] K. B. Fournier et al., Phys. Rev. Lett. 92, 165005 (2004). [5] C. A. Back et al., Phys. Rev. Lett. 87, 275003 (2001).

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