A technique is presented for reconstructing the height profiles of the volume emission rate and estimating the crosscut dimensions of rayed structures in auroras from the data of triangulation observations. A feature of the experimental data is the use of cameras that record radiation in a wide blue-green spectral range (380–580 nm) and a small distance between the cameras (4.12 km). The height profiles of the volume emission rate have been reconstructed for auroras with a pronounced rayed structure.
A Study of Rayed Structures in Auroras by Triangulation Methods: 1. Height Profiles of Volume Emission Rate
Cosmic Res
Cosmic Research ; 59 , 4 ; 223-230
2021-07-01
8 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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