Empirical model of variations in the helium 1083 nm emission. 2. Temperature

Details Empirical model of variations in the helium 1083 nm emission. 2. Temperature Empirical model of variations in the helium 1083 nm emission. 2. Temperature

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49..670s&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 5, pp.670-678

Physics

1

Ion Chemistry Of The Atmosphere

Scientific paper

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.

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