Experimental study on the full cycle evolution of high-intensity atmospheric dc arc discharge from breakdown to extinguishment

Ya-Hao Hu, Su-Rong Sun, Xian Meng, He-Ji Huang, and Hai-Xing Wang
Phys. Rev. E 109, 025205 – Published 6 February 2024

Abstract

In this study, the spatiotemporal evolution of full cycle of high-intensity dc argon arc discharge at atmospheric pressure is investigated by using a transferred arc device, which is easy to be directly observed in the experiment. Combining the voltage and current waveforms with high-speed images, the full cycle evolution process of high-intensity atmospheric dc arc can be divided into five different stages: breakdown pulse stage, cathode heating stage, current climbing stage, stable arc discharge stage, and finally arc extinguishing stage. The characteristics of each different stage are analyzed in detail through the electrical properties, high-speed pictures, and spectroscopic measurements. The results show that the strong luminescence region develops from the vicinity of cathode and anode to the middle in the breakdown pulse stage, which is explained from the spatiotemporal evolution of distributions of excited argon atom and ions. The development velocity of emission intensity of argon ions is mainly determined by the dominant stepwise ionization process. Then the cathode heating stage appears with many bright and nonuniformly distributed light spots on the cathode surface, and the electron emission mechanism of cathode gradually changes to the thermionic emission as the surface temperature rises. With the increase of arc current, the discharge channel significantly expands, then becomes stable due to the increment of the Lorentz force. The characteristics of arc extinguishing stage are clarified in terms of the decay of charged particles density.

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  • Received 17 March 2023
  • Accepted 4 January 2024

DOI:https://doi.org/10.1103/PhysRevE.109.025205

©2024 American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Authors & Affiliations

Ya-Hao Hu1,2, Su-Rong Sun1,*, Xian Meng2, He-Ji Huang2, and Hai-Xing Wang1,3,†

  • 1School of Astronautics, Beihang University, Beijing 100191, Beijing, China
  • 2Institute of Mechanics, Chinese Academy of Sciences, Beijing 100190, Beijing, China
  • 3Ningbo Institute of Technology, Beihang University, Ningbo 315800, Ningbo, China

  • *ssr18@buaa.edu.cn
  • whx@buaa.edu.cn

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Vol. 109, Iss. 2 — February 2024

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