Electron impact dissociative excitation of O2:: 1.: Kinetic energy distributions of fast oxygen atoms -: art. no. 5125

被引:13
|
作者
Makarov, OP [1 ]
Kanik, I [1 ]
Ajello, JM [1 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
atmospheres of Jovian satellites; analysis of Hubble Space Telescope UV observations; particle precipitation; electron impact dissociation cross sections; high-resolution UV spectroscopy; aurora and airglow of the Earth;
D O I
10.1029/2000JE001422
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[ 1] The kinetic energy distribution of oxygen atoms resulting from electron impact dissociation of O-2 has been measured. A high- resolution vacuum ultraviolet spectrometer was employed for the measurement of the OI( 115.2 nm, 130.4 nm, 135.6 nm) fine-structure emission line profiles at 35 eV and 100 eV electron impact energies. The deconvolved line profiles of atomic oxygen reveal the existence of a broad line profile (similar to 30 - 40 mAngstrom full width at half maximum) produced from a combination of dissociative excitation and dissociative ionization excitation processes. The atomic oxygen kinetic energy distributions at 100 eV electron impact energy spans the energy range from 1 to 10 eV, with a peak value near 1 eV. The excitation functions of OI( 115.2 nm, 130.4 nm, 135.6 nm) were measured in the vicinity of threshold, from 14 to 50 eV. The PACS classification is 34.80. Gs ( electron scattering- molecular dissociation) and 33.50Dq ( molecular spectra- fluorescence).
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页数:10
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