Breakdown of High-Pressure Gases in a Longitudinal Magnetic Field
It was discovered experimentally that a longitudinal magnetic field leads to an increase in the current density, conductivity, and partial energy input and a decrease in the times of the formation of all developments stages of discharge and transversal integral radiation and the channel expansion ra...
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| Veröffentlicht in: | High temperature 2019-03, Vol.57 (2), p.156-163 |
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| creator | Omarov, O. A. Omarova, N. O. Omarova, P. Kh Aliverdiev, A. A. |
| description | It was discovered experimentally that a longitudinal magnetic field leads to an increase in the current density, conductivity, and partial energy input and a decrease in the times of the formation of all developments stages of discharge and transversal integral radiation and the channel expansion rate. At the same time, a strong magnetic field displaces the maximum of spectral radiation density to the ultraviolet domain with the simultaneous generation of new spectral lines. Magnetic fields, which decrease the channel expansion rate and transversal radiation losses, increase the partial power, conductivity, and plasma temperature at the arc stages, which creates the conditions to obtain hot plasma and to develop the source of ultraviolet and X-ray radiations. |
| doi_str_mv | 10.1134/S0018151X19020159 |
| format | Article |
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A. ; Omarova, N. O. ; Omarova, P. Kh ; Aliverdiev, A. A.</creator><creatorcontrib>Omarov, O. A. ; Omarova, N. O. ; Omarova, P. Kh ; Aliverdiev, A. A.</creatorcontrib><description>It was discovered experimentally that a longitudinal magnetic field leads to an increase in the current density, conductivity, and partial energy input and a decrease in the times of the formation of all developments stages of discharge and transversal integral radiation and the channel expansion rate. At the same time, a strong magnetic field displaces the maximum of spectral radiation density to the ultraviolet domain with the simultaneous generation of new spectral lines. Magnetic fields, which decrease the channel expansion rate and transversal radiation losses, increase the partial power, conductivity, and plasma temperature at the arc stages, which creates the conditions to obtain hot plasma and to develop the source of ultraviolet and X-ray radiations.</description><identifier>ISSN: 0018-151X</identifier><identifier>EISSN: 1608-3156</identifier><identifier>DOI: 10.1134/S0018151X19020159</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Atoms and Molecules in Strong Fields ; Classical and Continuum Physics ; Industrial Chemistry/Chemical Engineering ; Laser Matter Interaction ; Line spectra ; Longitude ; Magnetic fields ; Materials Science ; Physical Chemistry ; Physics ; Physics and Astronomy ; Plasma Investigations ; Plasma temperature ; Ultraviolet spectra</subject><ispartof>High temperature, 2019-03, Vol.57 (2), p.156-163</ispartof><rights>Pleiades Publishing, Ltd. 2019</rights><rights>Copyright Springer Nature B.V. 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-36d26cbe8850748bca2cf88a00ab53a7192793af1131d4c82e83f287bce2538a3</citedby><cites>FETCH-LOGICAL-c316t-36d26cbe8850748bca2cf88a00ab53a7192793af1131d4c82e83f287bce2538a3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0018151X19020159$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0018151X19020159$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Omarov, O. 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Magnetic fields, which decrease the channel expansion rate and transversal radiation losses, increase the partial power, conductivity, and plasma temperature at the arc stages, which creates the conditions to obtain hot plasma and to develop the source of ultraviolet and X-ray radiations.</description><subject>Atoms and Molecules in Strong Fields</subject><subject>Classical and Continuum Physics</subject><subject>Industrial Chemistry/Chemical Engineering</subject><subject>Laser Matter Interaction</subject><subject>Line spectra</subject><subject>Longitude</subject><subject>Magnetic fields</subject><subject>Materials Science</subject><subject>Physical Chemistry</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Plasma Investigations</subject><subject>Plasma temperature</subject><subject>Ultraviolet spectra</subject><issn>0018-151X</issn><issn>1608-3156</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1kEFLxDAUhIMouK7-AG8Bz9W8pEnT47q4u0JFQQVvJU1fa9a1XZMW8d_bUsGDeHqHmW-YN4ScA7sEEPHVI2OgQcILpIwzkOkBmYFiOhIg1SGZjXI06sfkJIQtY0xKLmZkce3RvJXtZ0Pbim5c_Ro9eAyh90jXJmCgrqGGZm1Tu64vXWN29M7UDXbO0pXDXXlKjiqzC3j2c-fkeXXztNxE2f36drnIIitAdZFQJVe2QK0lS2JdWMNtpbVhzBRSmARSnqTCVMM3UMZWc9Si4jopLHIptBFzcjHl7n370WPo8m3b-6FPyDlPOFcqVmpwweSyvg3BY5XvvXs3_isHlo9L5X-WGhg-MWHwNjX63-T_oW8m2WjH</recordid><startdate>20190301</startdate><enddate>20190301</enddate><creator>Omarov, O. 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Magnetic fields, which decrease the channel expansion rate and transversal radiation losses, increase the partial power, conductivity, and plasma temperature at the arc stages, which creates the conditions to obtain hot plasma and to develop the source of ultraviolet and X-ray radiations.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0018151X19020159</doi><tpages>8</tpages></addata></record> |
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| subjects | Atoms and Molecules in Strong Fields Classical and Continuum Physics Industrial Chemistry/Chemical Engineering Laser Matter Interaction Line spectra Longitude Magnetic fields Materials Science Physical Chemistry Physics Physics and Astronomy Plasma Investigations Plasma temperature Ultraviolet spectra |
| title | Breakdown of High-Pressure Gases in a Longitudinal Magnetic Field |
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