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Empirical model of variations in the helium 1083 nm emission. 1. Intensity
Authors:N N Shefov  A I Semenov  O T Yurchenko
Institution:(1) Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences, Pyzhevskii per. 3, Moscow, 119017, Russia
Abstract:The model of variations in the orthohelium 1083 nm emission intensity has been constructed based on the measurements at different stations. The analytical approximations of the nighttime intensity variations depending on the phase age of the Moon, season, solar activity during the 11-year cycle, and geomagnetic disturbances are presented.
Keywords:
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