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dc.creatorVaranasi, P.en_US
dc.creatorChudamani, S.en_US
dc.date.accessioned2006-06-15T18:11:53Z
dc.date.available2006-06-15T18:11:53Z
dc.date.issued1988en_US
dc.identifier1988-RF-12en_US
dc.identifier.urihttp://hdl.handle.net/1811/17600
dc.description$^{\dag}$ Supported by the Planetary Atmospheres Branch of the Solar System Exploration Division of NASA under Grant-in-Aid No. NGR 33-015-139 and by the Upper Atmosphere Research Program of the Earth Sciences and Applications Division of NASA under Grant-in-Aid No. NAGW-1238.en_US
dc.descriptionAuthor Institution: Laboratory for Planetary Atmospheres Research, State University of New Yorken_US
dc.description.abstractUnless very careful and skillful precautions are taken, measurement of collision-induced line shifts using a tunable diode laser can be unreliable on account of the commonly encountered jitter and instability in the laser signal. However, when lines belonging to different molecules appear in the spectral scan as neighbors (reference lines) that do not interfere with the absorption of the observed line, as in the case of the three methanes and N2O, accurate line shift measurement is feasible. Using separate absorption cells for the reference and sample gases and placing them in series, we have been able to measure the pressure-induced shifts of the rotational lines of $^{12}CH_{4}, {^{13}}CH_{4}, {^{12}}CH_{3}D$ and $^{14}N_{2}O$ located between 1265 and $1275 cm^{-1}$. The temperature dependence of the shifts is also presented for collisions of the absorbers with $H_{2}, He, Ar, N_{2}, O$, and air.en_US
dc.format.extent163732 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titlePRESSURE SHIFT MEASUREMENTS ON THE INFRARED LINES OF $^{12}CH+_{4}, ^{13}CH_{4}, ^{12}CH_{3}D$ AND $^{14}N_{2}O$ AROUND $7.85 \mu m$ USING A TUNABLE DIODE LASER$^{\dag}$en_US
dc.typearticleen_US


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