FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1554489496> ?p ?o ?g. }

• W1554489496 endingPage "1162" @default.
• W1554489496 startingPage "1153" @default.
• W1554489496 abstract "Laser diagnostics at 266 nm were developed for the investigation of dense Z-pinch plasma at the 1 MA Zebra generator. A three-channel diagnostic can be configured as shadowgraphy and interferometry with two temporal frames or as a Faraday rotation polarimeter. Absorption and refraction of ultraviolet (UV) radiation in dense plasma is significantly smaller compared with regular diagnostics at the wavelength of 532 nm. Therefore, UV diagnostics allow direct investigation of the fine structure of the dense Z-pinch, development of instabilities, and a distribution of magnetic fields in Z-pinch plasma. Micropinches and instabilities with characteristic scales of 15-200 μm were observed in 1 MA wire-array Z pinches. Development of instabilities in wire-array Z pinches is in agreement with the magnetohydrodynamic simulations. Interferometry at the wavelength of 266 nm allows measurement of plasma density in the range (1-2)×10 <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>20</sup> cm <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>-3</sup> in the ablating wires, imploding plasma, stagnating pinch, and trailing material. A fast plasma motion was observed at the stagnation stage with two-frame shadowgraphy. Plasma motion at stagnation and prolonged implosion of trailing mass can provide the additional kinetic energy in the Z pinch and can be a source of enhanced X-ray radiation. A Faraday rotation diagnostic reveals a distribution of magnetic fields in the pinch and trailing material. The magnetic field strength and current were reconstructed from the rotation angles and phase shifts in plasma using the Abel transform. Current in the pinch can switch from the high-inductance neck and redistribute to the trailing material when resistance of peripheral plasma drops owing to heating by X-ray radiation. Further development of UV diagnostics to short wavelengths can help to apply well-established optical methods to Z-pinch plasma in multiMA pulsed power facilities." @default.
• W1554489496 created "2016-06-24" @default.
• W1554489496 creator A5033218423 @default.
• W1554489496 creator A5045776808 @default.
• W1554489496 creator A5064698313 @default.
• W1554489496 creator A5069451364 @default.
• W1554489496 creator A5072291891 @default.
• W1554489496 creator A5076771153 @default.
• W1554489496 creator A5086168607 @default.
• W1554489496 date "2014-05-01" @default.
• W1554489496 modified "2023-09-23" @default.
• W1554489496 title "UV Laser-Probing Diagnostics for the Dense Z Pinch" @default.
• W1554489496 cites W1885524789 @default.
• W1554489496 cites W1966958769 @default.
• W1554489496 cites W1967841226 @default.
• W1554489496 cites W1973189750 @default.
• W1554489496 cites W1984632716 @default.
• W1554489496 cites W1986329779 @default.
• W1554489496 cites W1988628294 @default.
• W1554489496 cites W1989654742 @default.
• W1554489496 cites W1996578252 @default.
• W1554489496 cites W2005949628 @default.
• W1554489496 cites W2007541516 @default.
• W1554489496 cites W2007771525 @default.
• W1554489496 cites W2009039712 @default.
• W1554489496 cites W2016263342 @default.
• W1554489496 cites W2023803760 @default.
• W1554489496 cites W2025145300 @default.
• W1554489496 cites W2030386972 @default.
• W1554489496 cites W2034523301 @default.
• W1554489496 cites W2039008529 @default.
• W1554489496 cites W2053320453 @default.
• W1554489496 cites W2055083044 @default.
• W1554489496 cites W2064100668 @default.
• W1554489496 cites W2064581101 @default.
• W1554489496 cites W2066075446 @default.
• W1554489496 cites W2076008627 @default.
• W1554489496 cites W2082722168 @default.
• W1554489496 cites W2083520018 @default.
• W1554489496 cites W2105343214 @default.
• W1554489496 cites W2126785048 @default.
• W1554489496 cites W2142252416 @default.
• W1554489496 cites W2143370988 @default.
• W1554489496 cites W2163500527 @default.
• W1554489496 cites W2328329970 @default.
• W1554489496 cites W2331110211 @default.
• W1554489496 doi "https://doi.org/10.1109/tps.2014.2314420" @default.
• W1554489496 hasPublicationYear "2014" @default.
• W1554489496 type Work @default.
• W1554489496 sameAs 1554489496 @default.
• W1554489496 citedByCount "11" @default.
• W1554489496 countsByYear W15544894962015 @default.
• W1554489496 countsByYear W15544894962016 @default.
• W1554489496 countsByYear W15544894962017 @default.
• W1554489496 countsByYear W15544894962018 @default.
• W1554489496 countsByYear W15544894962019 @default.
• W1554489496 countsByYear W15544894962020 @default.
• W1554489496 countsByYear W15544894962023 @default.
• W1554489496 crossrefType "journal-article" @default.
• W1554489496 hasAuthorship W1554489496A5033218423 @default.
• W1554489496 hasAuthorship W1554489496A5045776808 @default.
• W1554489496 hasAuthorship W1554489496A5064698313 @default.
• W1554489496 hasAuthorship W1554489496A5069451364 @default.
• W1554489496 hasAuthorship W1554489496A5072291891 @default.
• W1554489496 hasAuthorship W1554489496A5076771153 @default.
• W1554489496 hasAuthorship W1554489496A5086168607 @default.
• W1554489496 hasConcept C120665830 @default.
• W1554489496 hasConcept C121332964 @default.
• W1554489496 hasConcept C14480152 @default.
• W1554489496 hasConcept C146024833 @default.
• W1554489496 hasConcept C153385146 @default.
• W1554489496 hasConcept C166689943 @default.
• W1554489496 hasConcept C184779094 @default.
• W1554489496 hasConcept C185544564 @default.
• W1554489496 hasConcept C196046385 @default.
• W1554489496 hasConcept C2778260026 @default.
• W1554489496 hasConcept C2779824264 @default.
• W1554489496 hasConcept C31532427 @default.
• W1554489496 hasConcept C43503373 @default.
• W1554489496 hasConcept C520434653 @default.
• W1554489496 hasConcept C62520636 @default.
• W1554489496 hasConcept C82706917 @default.
• W1554489496 hasConceptScore W1554489496C120665830 @default.
• W1554489496 hasConceptScore W1554489496C121332964 @default.
• W1554489496 hasConceptScore W1554489496C14480152 @default.
• W1554489496 hasConceptScore W1554489496C146024833 @default.
• W1554489496 hasConceptScore W1554489496C153385146 @default.
• W1554489496 hasConceptScore W1554489496C166689943 @default.
• W1554489496 hasConceptScore W1554489496C184779094 @default.
• W1554489496 hasConceptScore W1554489496C185544564 @default.
• W1554489496 hasConceptScore W1554489496C196046385 @default.
• W1554489496 hasConceptScore W1554489496C2778260026 @default.
• W1554489496 hasConceptScore W1554489496C2779824264 @default.
• W1554489496 hasConceptScore W1554489496C31532427 @default.
• W1554489496 hasConceptScore W1554489496C43503373 @default.
• W1554489496 hasConceptScore W1554489496C520434653 @default.
• W1554489496 hasConceptScore W1554489496C62520636 @default.
• W1554489496 hasConceptScore W1554489496C82706917 @default.

• next