SPECTROSCOPY OF THE $O_{2}(b^{1}\Sigma^{+}_{g}-X^{3}\sigma^{-}_{g})$ ATMOSPHERIC BAND SYSTEM TO $v' =7$

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dc.creator Huestis, D. L. en_US
dc.creator Cosby, P. C. en_US
dc.creator Slanger, T. G. en_US
dc.creator Osterbrock, D. E. en_US
dc.date.accessioned 2006-06-15T15:47:50Z
dc.date.available 2006-06-15T15:47:50Z
dc.date.issued 1997 en_US
dc.identifier 1997-TG-03 en_US
dc.identifier.uri http://hdl.handle.net/1811/14090
dc.description $^{a}$H. D. Babcock and L. Herzberg, Astrophys. J. 108, 167 (1948). $^{b}$D. E. Osterbrock, et al., Pub. Astro. Soc. Of the Pacific 108, 277 (1996) $^{c}$T. G. Slanger, D. L. Huestis, D.E. Osterbrock, and J. P. Fulbright (submitted to Science, 1997). en_US
dc.description Author Institution: Molecular Physics Laboratory, SRI International; Observatories/Lick Observatory, University of California en_US
dc.description.abstract The Atmospheric Band System of $O_{2}$ has been extensively studied over many years. However, very few vibrational levels of the upper state are known. Some of the best data still come from Babcock and Herzberg’s solar absorption study, published in $1984^{a}$, for which the highest vibrational level is $v^{\prime} = 3$. In emission, vibrational levels up to $v^{\prime} = 5$ have been observed in aurora, but rotationally-resolved spectra from the atmosphere have been limited to $v^{\prime} = 0$, and specifically to the 0-1 band. New observations made with the Keck telescope and the HIRES echelle spectrograph ($0.34 cm^{-1}$ spectral resolution) on Mauna Kea show a wealth of nightglow emission data for the $O_{2}(b-X)$ transition, emanating from O-atom recombination at 90-100 km $altitude^{b,c}$. We have analyzed these rotationally-resolved bands extending to $v^{\prime} = 7 (\Delta v^{\prime} = 0,1)$ and expect to find bands from yet higher levels. Isotopic emissions in the 0-0 band at 762 nm are also observed. en_US
dc.format.extent 142184 bytes
dc.format.mimetype image/jpeg
dc.language.iso English en_US
dc.publisher Ohio State University en_US
dc.title SPECTROSCOPY OF THE $O_{2}(b^{1}\Sigma^{+}_{g}-X^{3}\sigma^{-}_{g})$ ATMOSPHERIC BAND SYSTEM TO $v' =7$ en_US
dc.type article en_US