2008
DOI: 10.1088/1009-0630/10/5/12
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Simulation to Predict Target Erosion of Planar DC Magnetron

Abstract: Plasma properties in a planar DC magnetron system are simulated by a non-selfconsistent particle method in two dimensions. Through tracing the trajectories of the energetic electrons in the specified electric field and the magnetic field, and treating the collision process by Monte Carlo method, the spatial profile of ionization events can be obtained conveniently. Assuming that the ions speed up from the ionization points and bombard the target with the energy at these points, and according to the Yamamura/Ta… Show more

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Cited by 5 publications
(2 citation statements)
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“…It is well known that the maximum target erosion depth profile takes place at points where θ = 0, i.e., the magnetic and electric fields are perpendicular [4,[16][17][18]. In balanced magnetron cathodes all points of the magnetic field lines where θ = 0 have the same value of r. However, in unbalanced magnetron cathodes these points where θ = 0 have different values of r. These experimental insights (see figure 4) are illustrated in figure 5.…”
Section: A Discharge Modelmentioning
confidence: 83%
“…It is well known that the maximum target erosion depth profile takes place at points where θ = 0, i.e., the magnetic and electric fields are perpendicular [4,[16][17][18]. In balanced magnetron cathodes all points of the magnetic field lines where θ = 0 have the same value of r. However, in unbalanced magnetron cathodes these points where θ = 0 have different values of r. These experimental insights (see figure 4) are illustrated in figure 5.…”
Section: A Discharge Modelmentioning
confidence: 83%
“…The maximum field strength on the surface of the target is about 0.05 T On the other hand, the strong magnetostatic field confines the electrons within the plasma. At magnetic fields of a few Tesla, the electrons typically have gyro radii of a few millimetres and tend to swirl above the target [28,29]. However, since their gyro radii are of the same order of magnitude as the characteristic length of the magnetic field, their orbits are not perfectly helical, though.…”
Section: Resultsmentioning
confidence: 99%