1986
DOI: 10.1016/0022-4073(86)90038-5
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Pressure broadening of methane lines in the 6190Åand 6825Åbands at room and low temperatures

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Cited by 27 publications
(9 citation statements)
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“…With our method of direct measurements of the rotational depopulation rates it is possible to obtain the depopulation rate coefficient of a well defined rovibrational level with a selected tetrahedral symmetry species A, E, F whereas, in line width measurements, the determination of the broadening coefficient for each tetrahedral component of a multiplet is not straightforward. Furthermore, for self-collisions, rotational depopulation rates can be measured at low temperature while the pressure above [15] which methane condenses is too low to measure pressure broadening accurately.…”
Section: Resultsmentioning
confidence: 99%
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“…With our method of direct measurements of the rotational depopulation rates it is possible to obtain the depopulation rate coefficient of a well defined rovibrational level with a selected tetrahedral symmetry species A, E, F whereas, in line width measurements, the determination of the broadening coefficient for each tetrahedral component of a multiplet is not straightforward. Furthermore, for self-collisions, rotational depopulation rates can be measured at low temperature while the pressure above [15] which methane condenses is too low to measure pressure broadening accurately.…”
Section: Resultsmentioning
confidence: 99%
“…For self-broadening, the only measurements performed at a temperature of 100 K are from Varanasi et al [14] for the R(0), R(1) and R(2) lines in the m 3 band and from Keffer et al [15] for unassigned lines of the 0.619 and 0.682 lm bands. For the R(0) line of m 3 , the self-broadening coefficient at 100 K is found to be (0.20 ± 0.02) cm À1 atm À1 that is close to the value obtained for 2m 3 though the upper vibrational states are different.…”
Section: Comparison With Broadening Coefficientsmentioning
confidence: 99%
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“…There have been numerous half-width measurements for transitions of 12 CH 4 with N 2 [24,[32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48][49]] O 2 , [32,42,44,45,48,49] air [32,36,38,40,42,43,45,[50][51][52][53], CH 4 [32,34,36,39,44,48,49,[54][55][56][57][58][59][60], and other molecules/atoms [32,…”
Section: Introductionmentioning
confidence: 99%