TY - JOUR
T1 - Fourier transform UV, visible, and infrared spectra of supersonically cooled CN radical
AU - Rehfuss, Breht D.
AU - Suh, Myeong Hyeon
AU - Miller, Terry A.
AU - Bondybey, Vladimir E.
PY - 1992/2
Y1 - 1992/2
N2 - The CN radical has been observed by Fourier transform spectroscopy in the ultraviolet, visible, and infrared regions of the spectrum. The radical was formed in a corona discharge of acetonitrile seeded in an inert carrier gas (helium or argon) at the throat of a pinhole nozzle and expanded into the vacuum chamber. The emission was resolved with a Bruker IFS-120 HR spectrometer. The B-X and A-X electronic transitions were observed from approximately 27 000 to 2500 cm-1. The B-X 0-0 band exhibited an anomalous rotational intensity distribution which cannot be described by a simple rotational temperature. This provides insight into the mechanisms of CN formation in our source. Vibrational levels up to v = 15 in both electronic states are observed. Such high vibrational excitation would require temperatures near 10 000 K. The population distribution appears nearly Boltzmann for low vibrational levels, albeit a high temperature, and deviates markedly at high vibrational levels.
AB - The CN radical has been observed by Fourier transform spectroscopy in the ultraviolet, visible, and infrared regions of the spectrum. The radical was formed in a corona discharge of acetonitrile seeded in an inert carrier gas (helium or argon) at the throat of a pinhole nozzle and expanded into the vacuum chamber. The emission was resolved with a Bruker IFS-120 HR spectrometer. The B-X and A-X electronic transitions were observed from approximately 27 000 to 2500 cm-1. The B-X 0-0 band exhibited an anomalous rotational intensity distribution which cannot be described by a simple rotational temperature. This provides insight into the mechanisms of CN formation in our source. Vibrational levels up to v = 15 in both electronic states are observed. Such high vibrational excitation would require temperatures near 10 000 K. The population distribution appears nearly Boltzmann for low vibrational levels, albeit a high temperature, and deviates markedly at high vibrational levels.
UR - http://www.scopus.com/inward/record.url?scp=36348968756&partnerID=8YFLogxK
U2 - 10.1016/0022-2852(92)90578-C
DO - 10.1016/0022-2852(92)90578-C
M3 - Article
AN - SCOPUS:36348968756
SN - 0022-2852
VL - 151
SP - 437
EP - 458
JO - Journal of Molecular Spectroscopy
JF - Journal of Molecular Spectroscopy
IS - 2
ER -