Numerical calculation of collision matrix in theory of molecular-line broadening and shift by gas pressure

V. A. Skvortsov

doi:10.1007/bf01038211

Numerical calculation of collision matrix in theory of molecular-line broadening and shift by gas pressure

Radiophysics and Quantum Electronics ◽

10.1007/bf01038211 ◽

1993 ◽

Vol 36 (9) ◽

pp. 654-657

Author(s):

V. A. Skvortsov

Keyword(s):

Numerical Calculation ◽

Gas Pressure ◽

Line Broadening ◽

Molecular Line

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A new semiclassical formulation for molecular line broadening

The Journal of Chemical Physics ◽

10.1063/1.452602 ◽

1987 ◽

Vol 86 (1) ◽

pp. 114-118 ◽

Cited By ~ 2

Author(s):

Jeanine Bonamy ◽

Georges Jolicard

Keyword(s):

Line Broadening ◽

Molecular Line

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Recent Results on Infrared Molecular Line Broadening and Shift Parameters

Remote Sensing of the Atmosphere for Environmental Security - NATO Security through Science Series ◽

10.1007/978-1-4020-5090-9_12 ◽

2007 ◽

pp. 185-201

Author(s):

Mary Ann H. Smith

Keyword(s):

Line Broadening ◽

Molecular Line

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Molecular-Gas-Pressure-Induced Line-Shift and Line-Broadening in the ν2-Band of H2S

Journal of Molecular Spectroscopy ◽

10.1006/jmsp.2002.8630 ◽

2002 ◽

Vol 216 (2) ◽

pp. 345-354 ◽

Cited By ~ 17

Author(s):

A Kissel ◽

B Sumpf ◽

H.-D Kronfeldt ◽

B.A Tikhomirov ◽

Yu.N Ponomarev

Keyword(s):

Gas Pressure ◽

Line Shift ◽

Molecular Gas ◽

Line Broadening

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A Self-Consistent Model Atmosphere Program with Applications to Solar 0I Resonance Lines

International Astronomical Union Colloquium ◽

10.1017/s0252921100151188 ◽

1970 ◽

Vol 2 ◽

pp. 65-84 ◽

Cited By ~ 2

Author(s):

R. Grant Athay ◽

Richard C. Canfield

Keyword(s):

Model Atmosphere ◽

Gas Pressure ◽

Line Broadening ◽

Consistent Model ◽

Self Consistent ◽

Good Agreement

AbstractProfiles and total intensities are computed for solar 01 resonance lines at λ1302 and λ1305 using a model atmosphere program that includes non-LTE effects in both hydrogen and oxygen and that includes microturbulence both as a line broadening mechanism and as a contribution to the gas pressure. Good agreement is obtained between computed and observed intensities. The computed profiles appear to have too much 'self-reversal.

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