The morphology of metallic ions in the upper atmosphere

Details The morphology of metallic ions in the upper atmosphere The morphology of metallic ions in the upper atmosphere

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85.6783k&link_type=abstract

Journal of Geophysical Research, vol. 85, Dec. 1, 1980, p. 6783-6801.

Mathematics

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7

Atmospheric Composition, Metal Ions, Spatial Distribution, Upper Atmosphere, Ion Density (Concentration), Iron, Solar Activity Effects

Scientific paper

Analysis of metallic ion data from a day-night pair of rockets, OGO 6, and the elliptic phases of AE-C and AE-D shows the presence of Fe(+) ions at altitudes above 400 km only at low magnetic latitudes. The detection probability of this ion decreases with altitude, with a maximum over the Atlantic and a minimum over India; the rocket data indicate ions in the E region during the day and on the bottom of the F layer at night. Mg(+) and Fe(+) are the dominant ions below 250 km at all latitudes, but Al(+), Na(+), Si(+), and Ca(+) are also detectable; a correlation was found between solar activity and metallic ion detection probability at low latitudes and high altitudes at night

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