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Solar zenith angle dependencies of F1-layer, <i>Nm</i>F2 negative disturbance, and G-condition occurrence probabilities

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Table 1. Average values of F1-layer and G condition percentage occurrences in latitude ranges 1–5 during the winter, summer, and spring and autumn months for the first (first number) and second (second number) half of the day for χ ≤ 90 ◦
Fig. 1. The dependence of the F1-layer percentage occurrences on the solar zenith angle in latitude range 1 (|8| ≤ 10 ◦ ) during the winter (solid lines), summer (dashed lines), and spring and autumn (dotted lines) months
Fig. 4. The dependence of the F1-layer (bottom panels), and G con- con-dition (top panels) probability functions on the solar zenith angle in latitude range 4 (45 ◦ &lt; |ϕ| ≤ 60 ◦ , 45 ◦ &lt; |8| ≤ 60 ◦ ) during the winter (solid lines), summer (dashed li
Fig. 5. The dependence of the F1-layer (bottom panels), and G con- con-dition (top panels) probability functions on the solar zenith angle in latitude range 5 (60 ◦ &lt; |8| ≤ 90 ◦ ) during the winter (solid lines), summer (dashed lines), and spring and au
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