journal article·2021-07-01Open access

Gas density distribution in a clustered-gas jet produced from a supersonic slit nozzle under high backing pressure

Huwang Xu, Guanglong Chen, D. N. Patel, Yunjiu Cao, Li Ren, Hongxia Xu, Huili Shao, Jianping He, Dong Eon Kim

AIP Advances· Volume 11· Issue 7

Abstract

A gas jet produced by adiabatic expansion of gas through a slit nozzle into a vacuum has been served as a target in the study of high harmonic generation or laser wakefield electron acceleration. In this work, Mach–Zehnder interferometry was utilized to obtain the gas density distribution in an argon cluster gas jet produced from a supersonic slit nozzle. The interference fringe distortion caused by the gas jet along the slit width under high backing pressure was recorded and inverted to a gas density profile. The gas backing pressure was up to 80 bars to obtain a gas jet with a higher density. It is found that the gas density in the jet is not uniform along the width direction of the slit nozzle and is the highest at the center of the jet. Along the gas jet, the highest gas density roughly decreases linearly. However, a steep density gradient is observed at P0 = 60–80 bars. Meanwhile, the highest gas density depends linearly on the gas backing pressure and the degree of dependence gradually decreases along the gas jet.
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Research context

OpenAlex topics: Laser-Plasma Interactions and Diagnostics · Laser-Matter Interactions and Applications · Laser-induced spectroscopy and plasma

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

School of Mathematics, Physics and Statistics, Shanghai University of Engineering Science 1 , Shanghai 201620, China

Department of Physics and Center for Attosecond Science and Technology, Pohang University of Science and Technology 2 , Pohang, Gyeongbuk 37673, South Korea

Max Planck POSTECH/KOREA Res. Init. 3 , Pohang, Gyeongbuk 37673, South Korea

School of Materials Engineering, Shanghai University of Engineering Science 4 , Shanghai 201620, China

Funding

National Natural Science Foundation of China · National Research Foundation of Korea

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