Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/101391
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Title: On a possible mechanism of space stem formation in negative long sparks
Authors: Zhao, X 
Popov, NA
Gan, Q
Ding, Y 
Du, Y 
He, J
Issue Date: 28-Jun-2023
Source: Geophysical research letters, 28 June 2023, v. 50, no. 12, e2023GL102834
Abstract: To study the mechanism of space stem formation, the high-speed direct imaging technique and Schlieren photography are used to simultaneously observe the space stems in a 1.35-m air gap under the lightning impulse voltage. It is found that the average length and diameter of the space stem is approximately 5 and 0.5 mm, which is about 1/3 of the length and 1/10 of the diameter of the local luminous region respectively. Moreover, the space stem exhibits a non-uniform distributed temperature with a maximum value of several hundred Kelvin for tens of microseconds. Accordingly, a possible mechanism is proposed that the space stem is formed at the primary corona streamer boundary as a result of the propagation of a secondary ionization wave from the HV electrode and survives long enough (to finish the polarization) due to the fast gas heating and production of atomic oxygen.
Publisher: Wiley-Blackwell
Journal: Geophysical research letters 
ISSN: 0094-8276
EISSN: 1944-8007
DOI: 10.1029/2023GL102834
Rights: © 2023. The Authors.
This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License (https://creativecommons.org/licenses/by-nc-nd/4.0/), which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.
The following publication Zhao, X., Popov, N. A., Gan, Q., Ding, Y., Du, Y., & He, J. (2023). On a possible mechanism of space stem formation in negative long sparks. Geophysical Research Letters, 50, e2023GL102834 is available at https://doi.org/10.1029/2023GL102834.
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