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In-Depth Information
0 0 0 0 0 0 0 0 0 0 0
8
8
7
7
e + O( 3 P)
6
6
5
5
4
4
O*(3p 3 P)
3
3
2
2
O * (3p 5 P)
1
1
0
0
0 0 0 0 0 0 0 0 0 0 0
Electron energy in eV
FIGURE 3.20 Electron excitation cross section of ground state atomic oxygen O( 3 P) into the
levels O(3p 3 P) and O(3p 5 P) in dependence on the electron energy according to the listed data
in [22]. (Data from Laher, R.R. and Gilmore, F.R., Updated excitation and ionization cross
section for electron and impact on atomic oxygen, Technical Report, R & D Associates Marina
Del Rey, CA, 1988.)
spectrum is influenced by many factors, e.g., the electron energy distribution function,
thedirectordissociativeexcitation,thecascadeprocesses,thebranching,theradiation
transport, and the collision of excited particle which may result in de-excitation
without radiation. All these factors have influence on the emission intensity, the
line broadening, or the ro-vibrational band structures of electronic transitions in
molecules. Generally, the quantum physics of the elementary excitation and de-
excitation processes and the collision-radiation model have to be involved to achieve
exactly the appropriate information from the measured emission spectrum for further
analysis.
Asanexample,theelectronimpactexcitationcrosssectionofatomicoxygenfrom
the ground state O( 3 P) into the levels O(3p 5 P) and O(3p 3 P) is shown in Figure 3.20
[22]. These states are the upper levels of the intensive optical transitions at 777 and
844 nm into the O(3s 5 S) and O(3s 3 S) state, respectively.
The optical emission cross section σ opt can be directly determined from measured
data in electron beam experiments according to (3.112) [20,23].
e
n gas ·
· s ·
γ s (
λ
) ·
R c
σ opt (
i
j
) =
I e ·
·
A s ·
F
(
λ, T
) ·
λ
(3.112)
L
·
c ·
γ c (
λ
) ·
R s
with I e the electron current, L path length of the electron beam, and n gas number
density.
The terms in the bracket describe the measured total photon flux per second
for the atomic transition i
j , with an effective radiation area of the standard
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