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Proceedings Paper

Modeling of the energy distribution of auroras
Author(s): N. N. Shefov; L. S. Evlashin; V. M. Ponomarev
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Paper Abstract

Spectral energy distribution of auroras at heights from 80 to 1000 km have been calculated on the base of global photometric model. It describes the processes of emission excitations by solar UV radiation and electron fluxes in auroral zone. This model deals with emissions from EUV to IR spectral regions (0.02 - 20 mcm) during night and day conditions. The main peculiarities of auroral spectra consist in spatial distribution of its components.

Paper Details

Date Published: 3 September 1997
PDF: 6 pages
Proc. SPIE 3237, 23rd European Meeting on Atmospheric Studies by Optical Methods, (3 September 1997); doi: 10.1117/12.284768
Show Author Affiliations
N. N. Shefov, Institute of Atmospheric Physics (Russia)
L. S. Evlashin, Polar Geophysical Institute (Russia)
V. M. Ponomarev, Institute of Atmospheric Physics (Russia)


Published in SPIE Proceedings Vol. 3237:
23rd European Meeting on Atmospheric Studies by Optical Methods
Vasily N. Ivchenko, Editor(s)

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