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dc.creatorAnderson, Richarden_US
dc.creatorSchearer, L. D.en_US
dc.creatorDowell, J. T.en_US
dc.creatorRainbow, Freden_US
dc.creatorSkipper, D. J.en_US
dc.date.accessioned2006-06-15T17:04:40Z
dc.date.available2006-06-15T17:04:40Z
dc.date.issued1973en_US
dc.identifier1973-K-07en_US
dc.identifier.urihttp://hdl.handle.net/1811/16036
dc.descriptionAuthor Institution: Department of Physics, University of Missourien_US
dc.description.abstractSeveral gases $CO_{2}, CO, CH_{4}, NO, SO_{2}, H_{2}O$, and $SiH_{4})$ have been added to a He flowing afterglow and the spectral emissions from the dissociation products have been observed from 3000 to 6000 \AA. $SiH_{4}$ gave the most interesting spectrum, with abundant Si lines of SiI and SiII, and bands of $SiH^{+}$ and SiH with the 4100 \AA SiH band being extremely intense. $SO_{2}$ did not give an abundant spectrum becaus the most intense emission of SO is below the region studied. In CO the comet tail emission of $CO^{+}$ was the principal emission with a few weak triplet emissions of CO. For $CO_{2}$ there was an intense comet tail emission of $CO^{+}$, the weak triplet emission of CO, and the intense many-band emission of Fox, Duffendack and Barker ‘s system of $CO_{2}$. Only the $\beta$ system of NO was observed along with lines of the $N_{2}$ second positive system. The 3064 \AA OH spectrum and the 3565 \AA $OH^{+}$ spectrum were observed with the addition of $H_{2}O$. With $CH_{4}$ both the 4300 and 3900 \AA systems of CH were observed.en_US
dc.format.extent186071 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleMOLECULAR SPECTRAL EMISSION FROM CASES ADDED TO A Hc FLOWING AFTERGLOWen_US
dc.typearticleen_US


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