Specific Features of the Longitudinal Distribution of Plasma Parameters in the Initial Segment of a Supersonic Jet Formed by a Pulsed Capillary Discharge
- Авторлар: Efimov A.V.1, Pashchina A.S.1, Chinnov V.F.1, Kazanskiy P.N.1
- 
							Мекемелер: 
							- Joint Institute for High Temperatures, Russian Academy of Sciences
 
- Шығарылым: Том 45, № 4 (2019)
- Беттер: 401-405
- Бөлім: Applied Physics
- URL: https://journal-vniispk.ru/1063-780X/article/view/187134
- DOI: https://doi.org/10.1134/S1063780X19040020
- ID: 187134
Дәйексөз келтіру
Аннотация
The paper presents the results of spectroscopic studies of the initial segment of a supersonic plasma jet formed by a pulsed discharge in a capillary made of carbon-containing polymer. Detection of the emission properties of the high-temperature core of the jet (the intensities and contours of the Hα and Hβ Balmer lines and the relative intensities of C II ion lines) with high temporal (1–50 μs) and spatial (30–50 μm) resolutions allowed the authors to reveal specific features of the longitudinal distributions of the electron density and temperature caused by the flow nonisobaricity along the initial segment of the supersonic jet.
Авторлар туралы
A. Efimov
Joint Institute for High Temperatures, Russian Academy of Sciences
							Хат алмасуға жауапты Автор.
							Email: axletter@gmail.com
				                					                																			                												                	Ресей, 							Moscow, 125412						
A. Pashchina
Joint Institute for High Temperatures, Russian Academy of Sciences
														Email: axletter@gmail.com
				                					                																			                												                	Ресей, 							Moscow, 125412						
V. Chinnov
Joint Institute for High Temperatures, Russian Academy of Sciences
														Email: axletter@gmail.com
				                					                																			                												                	Ресей, 							Moscow, 125412						
P. Kazanskiy
Joint Institute for High Temperatures, Russian Academy of Sciences
														Email: axletter@gmail.com
				                					                																			                												                	Ресей, 							Moscow, 125412						
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