Empirical model of variations in the helium 1083 nm emission. 1. Intensity

Details Empirical model of variations in the helium 1083 nm emission. 1. Intensity Empirical model of variations in the helium 1083 nm emission. 1. Intensity

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49...93s&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 1, pp.93-103

Physics

2

94.10.Fa

Scientific paper

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.

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