Characterization of transformer coupled oxygen plasmas by trace rare gases-optical emission spectroscopy and Langmuir probe analysis

Citation
Ncm. Fuller et al., Characterization of transformer coupled oxygen plasmas by trace rare gases-optical emission spectroscopy and Langmuir probe analysis, PLASMA SOUR, 9(2), 2000, pp. 116-127
Citations number
64
Categorie Soggetti
Physics
Journal title
PLASMA SOURCES SCIENCE & TECHNOLOGY
ISSN journal
09630252 → ACNP
Volume
9
Issue
2
Year of publication
2000
Pages
116 - 127
Database
ISI
SICI code
0963-0252(200005)9:2<116:COTCOP>2.0.ZU;2-#
Abstract
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.