UDC 551.510.535

Estimating the average energy of auroral electrons from 427.8 nm emission intensity measurements

Published в Solar-Terrestrial Physics · Volume 10, Issue 4, 2024 · Pages 65–71 · Rubrics: Results of current research
DOI 10.12737/stp-104202408
Received: 18.06.2024 Accepted: 02.09.2024 Published: 18.12.2024 Language of publication: ENG
Authors
1 Polar Geophysical Institute (302, nauchnyy sotrudnik)
from 01.01.1991 to 01.01.2022 Apatity, Murmansk, Russian Federation
2 Polar Geophysical Institute, RAS
Apatity, Russian Federation
We propose a method for estimating average energy of precipitating electrons from 427.8 nm emission intensity measurements. This method is based on the experimental dependence of the ratio of λ630.0 and λ427.8 nm emission intensities on the λ427.8 emission intensity and model calculations of the dependence of the average auroral electron energy on the I₆₃₀.₀/I₄₂₇.₈ ratio. We present numerical estimates of the influence of three factors on this dependence: the shape of the auroral electron energy spectrum, the atomic oxygen concentration, and the NO concentration. The dependence of the average energy of the auroral electron flux on the 427.8 nm emission intensity is obtained and its analytical approximation is presented.
auroras diagnostics average energy electron precipitation emission intensity 427.8 nm 630.0 nm
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