“…The summed flux density from of the two species was only slightly decreasing with increasing pressure up to about 8 mTorr, then a faster exponential decay occurred, characterized by a 50% decrease every 10 mTorr. The spatial distribution of the O − ion flux density was investigated in several works, which generally found a larger flux density near x e , corresponding to the largest plasma density or, equivalently, to the strongest magnetic field at the target [9,28,41]. It is difficult to extract quantitative trends, because the flux density distribution depends on the age of the target [9,42], the strength of the magnetic field in the magnetron [10], the type of excitation [9] (RF or DC), and energy-dispersive measurements are typically affected by the limited acceptance angle of the probe [9,15].…”