The NH radical is an extremely important specie in nitrogen chemical reaction networks, in the interstellar medium and atmospheric chemistry. Time resolved Fourier transform spectroscopy technique in the frequency range 10–13 µm has been applied for the measurement of a pure rotational spectrum of the NH free radical (NH) in the ground X3Σ− electronic state. Twelve high N (26–29) triplet-resolved pure rotation lines of NH were experimentally observed in the laboratory and compared with satellite ACE (Atmospheric Chemistry Experiment) solar data. In addition, discharge-generated vibration-rotation NH radical bands in the spectral range 1923–3571 cm−1 have been measured with a microsecond time resolution and spectral resolution of 0.02 cm−1. ...
Observations of ammonia in interstellar environments have revealed high levels of deuteration, and a...
High resolution solar spectra obtained from the ATMOS Fourier Transform Spectrometer (Spacelab 3 fli...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...
$^{1}$P. Hansen, M. Esplin, and H. Sakai, Paper presented at the 33rd Symposium of Molecular Spectro...
In this work we present a time-resolved FTIR spectroscopic study on kinetics of atomic and molecular...
Author Institution: CNRS, Laboratoire de Photophysique Mol\'eculaire, Universit\'e Paris SudFar infr...
$^{1}$S. D. Peyerimhoff and R. J. Buenker, Chemical Physics, 42, 167 (1979).Author Institution: Depa...
Author Institution: The J. Heyrovsky Institute of Physical Chemistry and Electrochemistry, Czechoslo...
Author Institution: NOAA Aeronomy Laboratory, R/E/AL2, 325 Broadway. Boulder, Colorado 80303; and Co...
Author Institution: Department of Chemistry, University of York, Heslington, York YO10 5DD, UK; Russ...
$^{1}$A.S. Pine, J. Opt. Soc. Am. 64, 1683 (1974), and 66, 97 (1976).The $\upsilon_{1}$ and $\upsilo...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...
none12siThe imidogen radical is an important molecule of the chemistry of nitrogen in the interstell...
Observations of ammonia in interstellar environments have revealed high levels of deuteration, and a...
Observations of ammonia in interstellar environments have revealed high levels of deuteration, and a...
High resolution solar spectra obtained from the ATMOS Fourier Transform Spectrometer (Spacelab 3 fli...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...
$^{1}$P. Hansen, M. Esplin, and H. Sakai, Paper presented at the 33rd Symposium of Molecular Spectro...
In this work we present a time-resolved FTIR spectroscopic study on kinetics of atomic and molecular...
Author Institution: CNRS, Laboratoire de Photophysique Mol\'eculaire, Universit\'e Paris SudFar infr...
$^{1}$S. D. Peyerimhoff and R. J. Buenker, Chemical Physics, 42, 167 (1979).Author Institution: Depa...
Author Institution: The J. Heyrovsky Institute of Physical Chemistry and Electrochemistry, Czechoslo...
Author Institution: NOAA Aeronomy Laboratory, R/E/AL2, 325 Broadway. Boulder, Colorado 80303; and Co...
Author Institution: Department of Chemistry, University of York, Heslington, York YO10 5DD, UK; Russ...
$^{1}$A.S. Pine, J. Opt. Soc. Am. 64, 1683 (1974), and 66, 97 (1976).The $\upsilon_{1}$ and $\upsilo...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...
none12siThe imidogen radical is an important molecule of the chemistry of nitrogen in the interstell...
Observations of ammonia in interstellar environments have revealed high levels of deuteration, and a...
Observations of ammonia in interstellar environments have revealed high levels of deuteration, and a...
High resolution solar spectra obtained from the ATMOS Fourier Transform Spectrometer (Spacelab 3 fli...
Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearin...