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Empirical model of variations in the helium 1083 nm emission. 2. Temperature
Authors:N. N. Shefov  A. I. Semenov  O. T. Yurchenko
Affiliation:1. Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences, Pyzhevskii per. 3, Moscow, 109017, Russia
Abstract:
Based on the measurements of the ortho helium 1083 nm emission intensity during twilights and on the calculation of its variations depending on the solar zenith angle, the method for determining the atmospheric temperature at heights of 300–1000 km during the nighttime period of day has been developed, taking into account the diurnal and seasonal conditions.
Keywords:
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