OH(AΣ+2) and rare gas-deuteride (NeD, ArD) excimers generated in microcavity plasmas: Ultraviolet emission spectra and formation kinetics

2007 ◽  
Vol 90 (20) ◽  
pp. 201504 ◽  
Author(s):  
B. J. Ricconi ◽  
S.-J. Park ◽  
S. H. Sung ◽  
P. A. Tchertchian ◽  
J. G. Eden
Keyword(s):  
Emission Spectra ◽  
Rare Gas ◽  
Ultraviolet Emission ◽  
Formation Kinetics

High-resolution far ultraviolet emission spectra of electron-excited molecular deuterium

1999 ◽  
Vol 32 (15) ◽  
pp. 3813-3838 ◽  
Author(s):  
H Abgrall ◽  
E Roueff ◽  
Xianming Liu ◽  
D E Shemansky ◽  
G K James
Keyword(s):  
High Resolution ◽  
Emission Spectra ◽  
Ultraviolet Emission ◽  
Far Ultraviolet

Emission Spectra of Deep Impurity States in Solid and Liquid Rare Gas Alloys

1972 ◽  
Vol 57 (11) ◽  
pp. 4628-4632 ◽  
Author(s):  
Ori Cheshnovsky ◽  
Baruch Raz ◽  
Joshua Jortner
Keyword(s):  
Emission Spectra ◽  
Rare Gas ◽  
Deep Impurity ◽  
Impurity States

Theoretical studies of vacuum ultraviolet emission spectra of NeLi+ and ArLi+

1991 ◽  
Vol 94 (5) ◽  
pp. 3707-3714 ◽  
Author(s):  
Suehiro Iwata ◽  
Shinkoh Nanbu ◽  
Hideki Kitajima
Keyword(s):  
Vacuum Ultraviolet ◽  
Emission Spectra ◽  
Theoretical Studies ◽  
Ultraviolet Emission

Ultraviolet Emission Spectra of Sunbeds¶

2002 ◽  
Vol 76 (6) ◽  
pp. 664 ◽  
Author(s):  
Beat Gerber ◽  
Patrick Mathys ◽  
Mirjana Moser ◽  
Dominique Bressoud ◽  
Charlotte Braun-Fahrländer
Keyword(s):  
Emission Spectra ◽  
Ultraviolet Emission

Emission spectra of group IV monohalide ions: , 3Π1–X1Σ+ emissions of SiBr+

1984 ◽  
Vol 62 (4) ◽  
pp. 353-360 ◽  
Author(s):  
M. Tsuji ◽  
K. Shinohara ◽  
S. Nishitani ◽  
T. Mizuguchi ◽  
Y. Nishimura
Keyword(s):  
Thermal Energy ◽  
Vibrational Temperature ◽  
Vibrational Analysis ◽  
Emission Spectra ◽  
Ionic Species ◽  
Group Iv ◽  
Rare Gas ◽  
Molecular Constants ◽  
Vibrational Levels ◽  
Effective Vibrational Temperature

Emission spectra of SiBr4 in the rare gas flowing afterglows have been measured to detect and identify SiBr+ emissions. Two systems of SiBr+ emissions were detected in the He, Ne, and Ar afterglows in the region from 335 to 380 nm. By analogy with the emission spectrum of SiCl+, they were ascribed to the [Formula: see text]–X1Σ+ and a3Π1–X1Σ+ subsystems of SiBr+. The vibrational analysis of the latter system gave the following molecular constants for the a3Π1 state: T0 = 29 140 ± 5 cm−1 and ΔG(1/2) = 392.0 ± 3.7 cm−1. The SiBr+ emissions disappeared when ionic species were removed from the afterglows, indicating that the emitting SiBr+ states were produced through thermal-energy reactions of rare gas ions with SiBr4. In the He and Ne afterglows, the [Formula: see text] ions were produced in higher vibrational levels than in the Ar afterglow. The relative vibrational populations in the He and Ne afterglows were nearly exponential with an effective vibrational temperature of 460 ± 30 K.

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