Empirical model of the OI 630 nm emission variations. 3. Emitting layer height

Details Empirical model of the OI 630 nm emission variations. 3. Emitting layer height Empirical model of the OI 630 nm emission variations. 3. Emitting layer height

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ge%26ae..47..750s&link_type=abstract

Geomagnetism and Aeronomy, Volume 47, Issue 6, pp.750-755

Physics

1

92.60.Hc

Scientific paper

The empirical model of variations in the emitting layer height and parameters has been developed based on an analysis of the rocket measurements of the vertical distributions in the 630 nm intensity. The dependences on the solar zenith angle during a day are most substantial. This dependence is responsible for the character of seasonal variations at different latitudes. The height of the emitting layer increases with increasing solar activity, reflecting a temperature rise in the upper atmosphere. The negative trend—0.35 km yr-1 in the interval 1964 1990—has been revealed.

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