2020
DOI: 10.1063/1.5135761
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Experimental observation and numerical investigation of filamentary structures in magnetized plasmas

Abstract: Filamentary structures in low-pressure, low-temperature plasmas are produced when strong magnetic fields are applied parallel to the electric field defined by parallel electrodes. Filamentary structures are regions within the plasma that have distinct properties such as optical brightness and extend along the magnetic field lines. In our experiments, an argon, radio frequency discharge is exposed to a strong background magnetic field in the magnetized dusty plasma experiment at Auburn University. Different for… Show more

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Cited by 9 publications
(13 citation statements)
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“…[ 24–29 ] Formation of these self‐organized patterns in low‐pressure magnetized plasmas (filamentation phenomenon) has been observed for over two decades. [ 24–29 ] These patterns are extended in the discharge along the magnetic axis, channelling from one sheath region to another. So far, filamentation phenomenon has been reported to appear at very low pressure (P20Pa) plasmas that are exposed to strong magnetic fields (B1T).…”
Section: Introductionmentioning
confidence: 99%
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“…[ 24–29 ] Formation of these self‐organized patterns in low‐pressure magnetized plasmas (filamentation phenomenon) has been observed for over two decades. [ 24–29 ] These patterns are extended in the discharge along the magnetic axis, channelling from one sheath region to another. So far, filamentation phenomenon has been reported to appear at very low pressure (P20Pa) plasmas that are exposed to strong magnetic fields (B1T).…”
Section: Introductionmentioning
confidence: 99%
“…The image sums up 500 frames of 8 μm diameter dust particles suspended in an argon plasma at a pressure, p = 16.6 Pa (125 mTorr), a radio frequency (rf) input power, P RF = 1.6 W, at 13.56 MHz, and a magnetic field of B = 2.5 T. The image reveals the competition between the previously reported dust gridding phenomenon (i.e., the rectangular grid pattern formed by the dust particle motion, shown as white lines in the image) [21][22][23] and the light grey, spiral structures observed in the visible light glow of the plasma (i.e., filamentary structures). [24][25][26][27][28][29] Therefore, in order to understand the dynamics of the dust particles in strongly magnetized plasmas, it is essential that we understand the underlying plasma dynamics. This paper is motivated by these observations and focuses on furthering the understanding of this pattern formation in the background plasma at high magnetic fields.…”
Section: Introductionmentioning
confidence: 99%
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