Auroral ionosphere: Comparison of time-dependent model with composition measurements
A time-dependent model of the auroral ionosphere including the odd nitrogen species, NO, N(/sup 2/D), and N (/sup 4/S), is used for comparison with data from a coordinated rocket-satellite measurement of an auroral event. The chemical scheme and the adopted rate coefficients have been shown to be compatible with daytime mid-latitude ionospheric chemistry. The electron flux and neutral atmospheric parameters measured on the satellite are used to compute the appropriate ionization and dissociation rates. The calculated NO/sup +/, O/sub 2//sup +/, O/sup +/, Ne, and NO densities agree well with the rocket measurements. The calculated N/sub 2//sup +/ densities are larger than the measured densities by a factor of 3 at most altitudes. The calculations show that the nitric oxide content of the aurora (approx.1.2 x 10/sup 9/ NO molecules/cm/sup 3/ at 105 km) is below the saturation value.
- Research Organization:
- Space Physics Research Laboratory, Department of Atmospheric and Oceanic Science University of Michigan, Ann Arbor, Michigan 48109
- OSTI ID:
- 5910342
- Journal Information:
- J. Geophys. Res.; (United States), Vol. 84:A8
- Country of Publication:
- United States
- Language:
- English
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GENERAL PHYSICS
AURORAE
IONIC COMPOSITION
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CHEMICAL REACTION KINETICS
DISSOCIATION
MOLECULAR IONS
NEON
NITROGEN
NUMERICAL SOLUTION
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ELEMENTS
FLUIDS
IONS
KINETICS
NONMETALS
PLANETARY IONOSPHERES
RARE GASES
REACTION KINETICS
640201* - Atmospheric Physics- Auroral
Ionospheric
& Magetospheric Phenomena