A comprehensive study of microwave (MW) activated CH 4 /H 2 /Ar plasmas used for diamond chemical vapor deposition is reported, focusing particularly on the effects of gross variations in the H 2 /Ar ratio in the input gas mixture (from H 2 /Ar mole fraction ratios of > 10:1, through to $1:99). Absolute column densities of C 2 (a) and CH(X) radicals and of H(n ¼ 2) atoms have been determined by cavity ringdown spectroscopy, as functions of height (z) above a substrate and of process conditions (CH 4 , H 2 , and Ar input mole fractions, total pressure, p, and input microwave power, P). Optical emission spectroscopy has also been used to explore the relative densities of electronically excited H atoms, and CH, C 2 , and C 3 radicals, as functions of these same process conditions. These experimental data are complemented by extensive 2D (r, z) modeling of the plasma chemistry, which provides a quantitative rationale for all of the experimental observations. Progressive replacement of H 2 by Ar (at constant p and P) leads to an expanded plasma volume. Under H 2-rich conditions, > 90% of the input MW power is absorbed through rovibrational excitation of H 2. Reducing the H 2 content (as in an Ar-rich plasma) leads to a reduction in the absorbed power density; the plasma necessarily expands in order to accommodate a given input power. The average power density in an Ar-rich plasma is much lower than that in an H 2-rich plasma operating at the same p and P. Progressive replacement of H 2 by Ar is shown also to result in an increased electron temperature, an increased [H]/[H 2 ] number density ratio, but little change in the maximum gas temperature in the plasma core (which is consistently $3000 K). Given the increased [H]/[H 2 ] ratio, the fast H-shifting (C y H x þ H $ C y H xÀ1 þ H 2 ; y ¼ 1À3) reactions ensure that the core of Ar-rich plasma contains much higher relative abundances of "product" species like C atoms, and C 2, and C 3 radicals. The effects of Ar dilution on the absorbed power dissipation pathways and the various species concentrations just above the growing diamond film are also investigated and discussed. V