2014
DOI: 10.1088/1009-0630/16/7/01
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Sheath Criterion for an Electronegative Plasma Sheath in an Oblique Magnetic Field

Abstract: The sheath criterion for an electronegative plasma composed of hot electrons, hot negative ions and cold positive ions in an oblique magnetic field is investigated. We discuss the effects of negative ions and external magnetic field on the sheath criterion. We find that the ion Mach number is of relatively low value because of Coulomb attraction between positive and negative ions. Also the ion Mach number depends on the magnitude and the angle of the magnetic field as well as the initial velocity of ion flow.

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Cited by 8 publications
(4 citation statements)
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“…In the past few decades, the study of plasma-surface transition in an electronegative plasma has become an area of interest both experimentally and theoretically [15][16][17][18][19][20]. The electrostatic potential distribution is a monotonic function in the sheath region.…”
Section: Introductionmentioning
confidence: 99%
“…In the past few decades, the study of plasma-surface transition in an electronegative plasma has become an area of interest both experimentally and theoretically [15][16][17][18][19][20]. The electrostatic potential distribution is a monotonic function in the sheath region.…”
Section: Introductionmentioning
confidence: 99%
“…A reduction in U 0z Min with increasing N N0 reveals that the negative ions help positive ions to enter the sheath region. Since a magnetized electronegative warm plasma has been visualized under the collisional environment, the values of U 0z Min are less than 1 for all the set of controlling parameters, consistent with [24,31], whereas U 0z Min takes values ⩾1 for collision-less plasmas consistent with [23,27].…”
Section: Resultsmentioning
confidence: 99%
“…The impact of an oblique magnetic field on the sheath structure in view of the positive ion Bohm speed has been investigated by several researchers [23][24][25][26][27] using the Sagdeev potential approach. However, they have neglected several imperative controlling parameters, such as those identified by Asserghine et al [23] in their model where they neglected the impact of collisions, ionization and adiabatic approximation, Yasserian and Aslaninejad [24] who neglected the impact of ionization, positive ion temperature, adiabatic approximation and non-extensivity of the system, Safa et al [25] who neglected the impact of collisions, ionization, adiabatic approximation, positive ion temperature and negative ions, Zou et al [26] who neglected the impact of collisions, ionization, positive ion temperature, adiabatic approximation, negative ions and non-extensivity of the system, and Huiping et al [27] who neglected the collisions, ionization, positive ion temperature, adiabatic approximation and non-extensivity of the system.…”
Section: Introductionmentioning
confidence: 99%
“…Besides these, it is crucial in the understanding of the Earthʼs ionosphere [16] and astrophysical plasmas [17]. In the past few decades, many works have been devoted to the study of plasma-sheath characteristics with two or more populations of negatively charged particles (e.g., two groups of electrons, or those containing negative ions) and this is still an attractive subject in plasma physics [18][19][20][21][22]. Sheridan et al [10] experimentally observed the existence of two-temperature groups: hot and cold electrons in magnetron sputtering plasma.…”
Section: Introductionmentioning
confidence: 99%