Line shape parameters of PH3 transitions in the Pentad near 4–5μm: Self-broadened widths, shifts, line mixing and speed dependence

2014 ◽  
Vol 302 ◽  
pp. 17-33 ◽  
Author(s):  
V. Malathy Devi ◽  
D. Chris Benner ◽  
Isabelle Kleiner ◽  
Robert L. Sams ◽  
Leigh N. Fletcher
Keyword(s):  
Line Shape ◽  
Shape Parameters ◽  
Speed Dependence ◽  
Line Mixing

Dicke narrowing, speed dependence and line mixing of self-broadened CO2 absorption lines in the 30013 ← 00001 band. Measurements and line shape testing

2021 ◽  
Vol 34 (5) ◽  
pp. 334-342
Author(s):  
V.A. Kapitanov ◽  
K.Yu. Osipov ◽  
A.E. Protasevich ◽  
Yu.N. Ponomarev ◽  
Ya.Ya. Ponurovskii
Keyword(s):  
Line Shape ◽  
Absorption Lines ◽  
Speed Dependence ◽  
Line Mixing

LINE SHAPE PARAMETERS OF WATER VAPOR TRANSITIONS IN THE 3645-3975 cm−1 REGION

2017 ◽  
Author(s):  
Mary Smith ◽  
Thomas Blake ◽  
Robert Sams ◽  
Candice Renaud ◽  
Bastien Vispoel ◽  
...  
Keyword(s):  
Water Vapor ◽  
Line Shape ◽  
Shape Parameters

scholarly journals Line-shape parameters for the first rotational lines of HD in He

2020 ◽  
Vol 19 ◽  
pp. 100063 ◽  
Author(s):  
Franck Thibault ◽  
Raúl Z. Martínez ◽  
Dionisio Bermejo ◽  
Piotr Wcisło
Keyword(s):  
Line Shape ◽  
Shape Parameters

scholarly journals Fully quantum calculations of the line-shape parameters for the Hartmann-Tran profile: A CO-Ar case study

2020 ◽  
Vol 243 ◽  
pp. 106803 ◽  
Author(s):  
Grzegorz Kowzan ◽  
Piotr Wcisło ◽  
Michał Słowiński ◽  
Piotr Masłowski ◽  
Alexandra Viel ◽  
...  
Keyword(s):  
Line Shape ◽  
Quantum Calculations ◽  
Shape Parameters

THE SHAPES OF PHOTOELECTRON SATELLITE SPECTRA

2002 ◽  
Vol 09 (02) ◽  
pp. 1209-1212 ◽  
Author(s):  
V. G. YARZHEMSKY ◽  
V. I. NEFEDOV ◽  
M. YA. AMUSIA ◽  
L. V. CHERNYSHEVA
Keyword(s):  
Line Shape ◽  
Shape Parameters ◽  
Line Shapes ◽  
Peak Structure ◽  
Experimental Line

Line shapes of photoionization satellites are theoretically investigated. Calculations were carried out for the satellite states 1s2s(3S)3s(2S) and 3s3p5(1P)4s(2P) of Ne 1s and Ar 3p vacancies, respectively, created in photoionization. Theory excellently reproduces experimental line shape parameters of the first satellite and predicts the two-peak structure of the second.

Sign in / Sign up

Export Citation Format

Share Document