On I(5577 Å) and I (7620 Å) auroral emissions and atomic oxygen densities
Autor: | E. J. Llewellyn, A. Vallance Jones, R. L. Gattinger |
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Jazyk: | angličtina |
Rok vydání: | 1996 |
Předmět: |
Atmospheric Science
Materials science lcsh:QC801-809 Geology Astronomy and Astrophysics Electron lcsh:QC1-999 lcsh:Geophysics. Cosmic physics Space and Planetary Science Ionization Excited state Earth and Planetary Sciences (miscellaneous) Light emission lcsh:Q Pitch angle Atomic physics Thermosphere lcsh:Science Electron ionization Excitation lcsh:Physics |
Zdroj: | Annales Geophysicae, Vol 14, Pp 687-698 (1996) Annales Geophysicae, Vol 14, Iss 7, Pp 687-698 (0000) |
ISSN: | 1432-0576 0992-7689 |
Popis: | A model of auroral electron deposition processes has been developed using Monte Carlo techniques to simulate electron transport and energy loss. The computed differential electron flux and pitch angle were compared with in situ auroral observations to provide a check on the accuracy of the model. As part of the energy loss process, a tally was kept of electronic excitation and ionization of the important atomic and molecular states. The optical emission rates from these excited states were computed and compared with auroral observations of η(3914 Å), η(5577 Å), η(7620 Å) and η(N2VK). In particular, the roles played by energy transfer from N2(A3Σ+u) and by other processes in the excitation of O(1S) and O2(b1Σ+g) were investigated in detail. It is concluded that the N2(A3Σ+u) mechanism is dominant for the production of OI(5577 Å) in the peak emission region of normal aurora, although the production efficiency is much smaller than the measured laboratory value; above 150 km electron impact on atomic oxygen is dominant. Atomic oxygen densities in the range of 0.75±0.25 MSIS-86 [O] were derived from the optical comparisons for auroral latitudes in mid-winter for various levels of solar and magnetic activity. |
Databáze: | OpenAIRE |
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