Infrared photons from the radiative cascade accompany both the gas phase NO2 continuum chemiluminescence (which originates from its 2B2 and 2B1 states) and the NO beta bands. When these upper electronic states are excited by recombination/desorption at surfaces of low Earth orbiting spacecraft, similar IR emission spectrums will be observed. The principal NO2 features (other than the long wavelength tail of its electronic transitions) are the nu sub 3 fundamental sequence near 6.2 microns and nu sub 1 + nu sub 3 intercombination bands near 3.6 microns; NO would emit the delta v=1 and delta v=2 systems above 5.3 and 2.7 microns. Because of the long radiative lifetimes of the upper vibrational states, the infrared radiances in projections par...
Time resolved Fourier transform infrared emission has been used to study the photolysis of NO2 and i...
Recent work suggested that NO2 may be responsible for the observed continuum glow near surfaces of t...
Author Institution: Laboratoire de Physique, Mol\'eculaire et d'Optique Atmosph\'erique C N R S B\^{...
Experiments on formation and excitation of NO2 and NO molecules at (and near) laboratory surfaces of...
Infrared emission from the low-pressure gas-phase NO — О reaction system has been studied from 1 to ...
Infrared chemiluminescence from the process O + NO (+M) NO2 + hv (+M) has been studied between 1.3 a...
Author Institution: Concord Radiance Laboratory Utah State University, Bedford, Massachusetts; Air F...
Author Institution: Department of Chemistry, University of PennsylvaniaLaser excitation of the $NO_{...
The infrared radiation over the range from 4 to 1000 microns from atoms and molecules in the earth's...
The 248 nm photolysis of NO2 results in an inverted vibrational distribution in NO(v) which agrees w...
to measure infrared emission spectra from the earth limb atmosphere. Spectrometers measured emission...
The spectroscopy of the υ = 1 → υ = 0 fundamental vibration-rotation band of nitric oxide (NO) in Ea...
Collisional quenching of NO A(2)Σ(+) (v = 0, 1) by O2 has been studied through the detection of vibr...
Although only a minor constituent of the earth's upper atmosphere, nitric oxide (NO) plays a major r...
This thesis presents the study of a selection of gas phase chemical processes using time-resolved Fo...
Time resolved Fourier transform infrared emission has been used to study the photolysis of NO2 and i...
Recent work suggested that NO2 may be responsible for the observed continuum glow near surfaces of t...
Author Institution: Laboratoire de Physique, Mol\'eculaire et d'Optique Atmosph\'erique C N R S B\^{...
Experiments on formation and excitation of NO2 and NO molecules at (and near) laboratory surfaces of...
Infrared emission from the low-pressure gas-phase NO — О reaction system has been studied from 1 to ...
Infrared chemiluminescence from the process O + NO (+M) NO2 + hv (+M) has been studied between 1.3 a...
Author Institution: Concord Radiance Laboratory Utah State University, Bedford, Massachusetts; Air F...
Author Institution: Department of Chemistry, University of PennsylvaniaLaser excitation of the $NO_{...
The infrared radiation over the range from 4 to 1000 microns from atoms and molecules in the earth's...
The 248 nm photolysis of NO2 results in an inverted vibrational distribution in NO(v) which agrees w...
to measure infrared emission spectra from the earth limb atmosphere. Spectrometers measured emission...
The spectroscopy of the υ = 1 → υ = 0 fundamental vibration-rotation band of nitric oxide (NO) in Ea...
Collisional quenching of NO A(2)Σ(+) (v = 0, 1) by O2 has been studied through the detection of vibr...
Although only a minor constituent of the earth's upper atmosphere, nitric oxide (NO) plays a major r...
This thesis presents the study of a selection of gas phase chemical processes using time-resolved Fo...
Time resolved Fourier transform infrared emission has been used to study the photolysis of NO2 and i...
Recent work suggested that NO2 may be responsible for the observed continuum glow near surfaces of t...
Author Institution: Laboratoire de Physique, Mol\'eculaire et d'Optique Atmosph\'erique C N R S B\^{...