chemical physics of discharges - Argonne National Laboratory
chemical physics of discharges - Argonne National Laboratory chemical physics of discharges - Argonne National Laboratory
1.0 I - a. I n TEMPERATURE - OK Figure 3 Equilibrium conposition of equimolar CH&-N* mixture. (a) Including solid carbon; (b) Excluding solid carbor.. Region above T, common. I 0 70 60 x) 40 30 20 IO NITROGEN GONVCRSK)N 0 10-1 2 5 100 2 5 IO' 2 5 P41'IW - - Fig'xe 4 yieid cf HCI:, expressed as percent Pi2 converted, as a function of input stoichiometry. Solid lines shov .win-- yield predicted by thermodynaniic equilibriwn. Lata points shov experimental results frx. the plas-a reactcr: ~r flow rate 42 std cc/sec,. total reagent flow rate 2 std cc/sec, net pmer - 3.5 kv. Reactor pressure identified with key. Points labeled x from plasma Jet studies6J7.
352 appeared in the literature. O'Halloran, et al?', have directly sampled an argon plasma jet using a specially designed entrance cone opening to a time-of-flight mass spectrometer. Raisen, et a1.21J have made spectroscopic identifications of species in an air plasma. Unlike the mass spectrometer measurements, however, emission spectroscopy 1s difficult to quantify due to the wide variance in the oscillator-strengths of the likely emitters. I Faced with the difficulty of determining plasma composition directly, one is prone to apply equilibrium predictions as 8 guide to local plasma composition. Referring both to Figs. 2 and 3, a highly dissociated composition can be expected in most of the plasm region. Temperatures in excess of 10,000 K, expected over most of the central region of the plasma, would dictate that the atomic species H, C, and N, and their ions would predominate. QUENCHING At this juncture it is important to ask what Changes in composition would be encountered on cooling the €I-C-N atom plasma. A slow, gradual cooling of the labile intermediates resident in the plasma zone may well allow the system to revert to the original reactants along an equilibrium path. Kroepelin and Kippid2 found tNs effect in their study of a 10 amp, 40 volt d.c. arc burning in 8 hydro- carbon-nitrogen atmosphere. The composition of the slowly cooled arc-heated gases was found to be mainly w, &, and C1 and C2 hydrocarbons. No HCN was observed. Under extremely rapid cooling, however, kinetic limitations can interpose along the reaction path to yield different, uwre interesting or valuable products. The Cold-Wall Tube. A small-diameter, water-cooled tube was selected from the variaty of available high-cooling-rate devices, to provide rapid and convenient quenching of the plasm species. Figure lb shows a diagram of the simple design of the three-concentric tube arrangement of the quenching probe23. The overall outside diameter of the probe was 318 in. The internal diameter of the quenching tube which receives the hot plasma was 0.032 in. The surfaces of the inner tube were stainless steel; other parts were fabricated from copper. The effect of a variation in the composition of the cold surface waa not studied. Cooling Rate. Due to the Ngh rate of heat transfer from plasma to adjacent cold wall, rapid cooling occurs in the quenching tube. Freeman and ~ltrivan~~,~5 have measured an initial temperature decay rate of 5 x 107 Vsec in water-cooled tubes. In their model of the heat-transfer process occurring in very smaU tubes, Anmann and Timminsm have calculated cooling rates greater than lo9 Vsec. *obably quenching rates in this range were associated with the quenching tube used in. this study. Reaction Path During Quench. Unfortunately, there is a sparsity of hightemperature kinetic data for the H-C-N system. Hence one is unable to predict with certainty the reaction path followed as the atomic species H, C, and N, are cooled from 15,000 K to 500 K in 10 11tI~iBeCOnd6, for example. After an examination of
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352<br />
appeared in the literature. O'Halloran, et al?', have directly sampled an argon<br />
plasma jet using a specially designed entrance cone opening to a time-<strong>of</strong>-flight<br />
mass spectrometer. Raisen, et a1.21J have made spectroscopic identifications <strong>of</strong><br />
species in an air plasma. Unlike the mass spectrometer measurements, however,<br />
emission spectroscopy 1s difficult to quantify due to the wide variance in the<br />
oscillator-strengths <strong>of</strong> the likely emitters.<br />
I<br />
Faced with the difficulty <strong>of</strong> determining plasma composition directly, one is<br />
prone to apply equilibrium predictions as 8 guide to local plasma composition.<br />
Referring both to Figs. 2 and 3, a highly dissociated composition can be expected<br />
in most <strong>of</strong> the plasm region. Temperatures in excess <strong>of</strong> 10,000 K, expected over<br />
most <strong>of</strong> the central region <strong>of</strong> the plasma, would dictate that the atomic species<br />
H, C, and N, and their ions would predominate.<br />
QUENCHING<br />
At this juncture it is important to ask what Changes in composition would be<br />
encountered on cooling the €I-C-N atom plasma. A slow, gradual cooling <strong>of</strong> the<br />
labile intermediates resident in the plasma zone may well allow the system to<br />
revert to the original reactants along an equilibrium path.<br />
Kroepelin and Kippid2<br />
found tNs effect in their study <strong>of</strong> a 10 amp, 40 volt d.c. arc burning in 8 hydro-<br />
carbon-nitrogen atmosphere. The composition <strong>of</strong> the slowly cooled arc-heated gases<br />
was found to be mainly w, &, and C1 and C2 hydrocarbons. No HCN was observed.<br />
Under extremely rapid cooling, however, kinetic limitations can interpose along<br />
the reaction path to yield different, uwre interesting or valuable products.<br />
The Cold-Wall Tube. A small-diameter, water-cooled tube was selected from<br />
the variaty <strong>of</strong> available high-cooling-rate devices, to provide rapid and convenient<br />
quenching <strong>of</strong> the plasm species. Figure lb shows a diagram <strong>of</strong> the simple design<br />
<strong>of</strong> the three-concentric tube arrangement <strong>of</strong> the quenching probe23. The overall<br />
outside diameter <strong>of</strong> the probe was 318 in. The internal diameter <strong>of</strong> the quenching<br />
tube which receives the hot plasma was 0.032 in. The surfaces <strong>of</strong> the inner tube<br />
were stainless steel; other parts were fabricated from copper. The effect <strong>of</strong> a<br />
variation in the composition <strong>of</strong> the cold surface waa not studied.<br />
Cooling Rate. Due to the Ngh rate <strong>of</strong> heat transfer from plasma to adjacent<br />
cold wall, rapid cooling occurs in the quenching tube. Freeman and ~ltrivan~~,~5<br />
have measured an initial temperature decay rate <strong>of</strong> 5 x 107 Vsec in water-cooled<br />
tubes. In their model <strong>of</strong> the heat-transfer process occurring in very smaU tubes,<br />
Anmann and Timminsm have calculated cooling rates greater than lo9 Vsec. *obably<br />
quenching rates in this range were associated with the quenching tube used<br />
in. this study.<br />
Reaction Path During Quench. Unfortunately, there is a sparsity <strong>of</strong> hightemperature<br />
kinetic data for the H-C-N system. Hence one is unable to predict with<br />
certainty the reaction path followed as the atomic species H, C, and N, are cooled<br />
from 15,000 K to 500 K in 10 11tI~iBeCOnd6, for example. After an examination <strong>of</strong>