Author:
Mangina Rao S.,Ajello Joseph M.,West Robert A.,Dziczek Dariusz
Abstract
ABSTRACT
Electron-impact emission cross sections for N2 were measured in the
wavelength range of 330–1100 nm at 25 eV and 100 eV impact energies. Cross
sections of several molecular emission bands of the first positive band system
B
3Π
g
+(ν′) → A
3Σ
g
+(ν″) and the second
positive band system C
3Π
u
(ν′) → B
3Π
g
(ν″) of N2, the first
negative band (1NB) system B
2Σ
u
+(ν′) → X
2Σ
g
+(ν″) and Meinel band
system A
2Π
u
(ν′) → X
2Σ
g
+(ν″) of
N2
+ ions as well as line emissions of N (N i)
and N+ (N ii) in the visible–optical–near-IR wavelength
range reported in this work were measured for the first time in a single
experimental setup at high spectral resolving power (λ/Δλ ≈ 10000) under
single-collision-scattering geometry and optically thin conditions. Rotational
emission lines of N2 and N2
+ were observed for
strong emission bands at a gas temperature of about 300 K. The absolute cross
section of the strongest (0,0) vibrational band at 391.43 nm of 1NB was
determined using the standard Hα emission cross sections of
H2 by electron impact at both 25 eV and 100 eV electron-impact
energies, and the cross sections for the remainder of the emissions were
determined using (0,0) 1NB value. A comparison of the present emission cross
sections with the earlier published data from both electron energy loss and
electron-impact-induced fluorescence emission is discussed.
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
24 articles.
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