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

被引:126
作者
Fuller, NCM
Malyshev, MV
Donnelly, VM
Herman, IP
机构
[1] Bell Labs, Lucent Technol, Murray Hill, NJ 07974 USA
[2] Columbia Univ, Columbia Radiat Lab, Dept Appl Phys, New York, NY 10027 USA
关键词
D O I
10.1088/0963-0252/9/2/304
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Trace rare gases-optical emission spectroscopy (TRG-OES) and Langmuir probe analysis have been used to measure the electron temperature, T-e, in a high-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 rare gas actinometry (Ar, 7504 Angstrom). In the H-(inductive)-mode, T-e increases from 2.6 to 3.4 eV for the low-energy electrons sampled by the Langmuir probe and from similar to 3.5 to 6.0 eV for the high-energy electrons sensed 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 power 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 lowest 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 distribution 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 low 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 to the high rate of O-atom recombination on the mostly stainless-steel walls. A detailed accounting of the sources of O (8446 Angstrom) emission revealed significant contributions from electron impact excitation from O(S-1) and dissociative excitation of O-2.
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页码:116 / 127
页数:12
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