Computer Science – Sound
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36..621z&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 36, June 1988, p. 621-628.
Computer Science
Sound
18
F Region, Gas Dissociation, Ionospheric Electron Density, Oxygen Ions, Plasma Spectra, Recombination Coefficient, Airglow, Gas Temperature, Rocket Sounding, Vibrational Spectra
Scientific paper
The rate coefficient for the excitation of the O(1S) state due to the dissociative recombination of O2(+) (v of not greater than 3) ions has been determined as a function of the electron temperature from 300-3500 K. In agreement with the work of Guberman (1987), the results suggest that the absolute magnitude of alpha(1S) is nearly the same for a wide variety of O2(+) vibrational distributions over the electron temperature range normally encountered in the nocturnal F-region. It is noted that previous studies which modeled 5577-A airglow data using a fixed value for f(1S) may be misleading.
No associations
LandOfFree
The excitation of the O(1S) state by the dissociative recombination of O2(+) ions - Electron temperature dependence does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The excitation of the O(1S) state by the dissociative recombination of O2(+) ions - Electron temperature dependence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The excitation of the O(1S) state by the dissociative recombination of O2(+) ions - Electron temperature dependence will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1183033