NASA NTRS · 19720015735
The ionosphere above Alma Ata during a solar eclipse
Abstract
The eclipse effect was manifested during the second phase: the ionization of the F1- and F2-layers decreased and the minimum effective heights of E and F2 increased due to recombination processes. The manner in which electron density is distributed over the levels was ascertained from analysis of N(t) curves.
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Rudina, M. P., Kozina, P. Y.. 1972-05-01. The ionosphere above Alma Ata during a solar eclipse. https://ntrs.nasa.gov/citations/19720015735
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