Trace rare gases-optical emission spectroscopy (TRG-OES) and Langmuir probe
analysis have been used to measure the electron temperature, T-e, in a hig
h-density inductively (transformer) coupled (TCP) 10 mTorr oxygen plasma as
a function of the 13.56 MHz radio frequency (rf) power. The oxygen atomic
densities were estimated by O-atom optical emission (8446 Angstrom), and ra
re gas actinometry (Ar, 7504 Angstrom). In the H-(inductive)-mode, T-e incr
eases from 2.6 to 3.4 eV for the low-energy electrons sampled by the Langmu
ir probe and from similar to 3.5 to 6.0 eV for the high-energy electrons se
nsed by TRG-OES as the rf power is increased from 120 to 1046 W. In the E-(
capacitive)-mode, below 50 W, T-e measured by TRG-OES increases with rf pow
er from similar to 4 eV at very low power (similar to 7 W) to similar to 6.
1 eV at 45 W. Between the highest E-mode power (similar to 50 W) and lowes
t H-mode power (similar to 120 W), the T-e measured by TRG-OES drops from 6
.1 to 3.5 eV, while T-e derived from Langmuir probe measurements drops only
slightly from 3.0 to 2.6 eV. In the H-mode, the electron energy distributi
on function (EEDF) is bi-Maxwellian from similar to 120 to 1046 W. In the E
-mode, the EEDF changes from nearly Maxwellian (possibly Druyvesteyn) at lo
w rf powers (similar to 7 W) to bi-Maxwellian at the higher E-mode powers (
similar to 45 W). O-2 dissociation is low (similar to 2%) at the maximum rf
power density of 5.7 W cm(-2) (1046 W), and this low value is attributed t
o the high rate of O-atom recombination on the mostly stainless-steel walls
. A detailed accounting of the sources of O (8446 Angstrom) emission reveal
ed significant contributions from electron impact excitation from O(S-1) an
d dissociative excitation of O-2.