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Maximum ion density, a condition that makes for efficient radio transmission, occurs within two sublayers: the lower E region, which exists from 90 to 120 km (about 55 to 75 miles) in altitude; and the F region, which exists from 150 to 300 km (about 90 to 185 miles) in altitude.
The local time spread of the daytime maximum ion density increases with increase in solar activity.
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As it was shown in "The 8 9 October 2012 magnetic storm and the position of the auroral oval and of the westward auroral electrojet" section, the maximum of the ion density and the most equatorial boundary of the westward auroral electrojet were located at the same magnetic latitude in dipole approximation.
The F region has two maxima (i.e., two periods of highest ion density) during daylight hours, called F1 and F2.
For example, the lithium ion density at r = 10 m (solid line) is maximum approximately at 106 cm−3 at 4 ms after the release, and it becomes less than 102 cm−3 within 1 s after the release.
Statistical analyses of the ion density data at 1100 km altitude during the solar maximum of cycle 21 have revealed that the H+ density has negative correlation with the solar flux F10.7 while O+ has positive correlation.
However, in order to get the maximum ion flux per unit membrane area it is desirable to operate at the highest possible current density.
It is found that maximum irregularity intensity is obtained in the geomagnetic latitude range of 10 20° for both electron density and ion density.
ion density.
(c) Solar wind ion density and reflected ion density.
Figure 1 a d show the C/NOFS orbit, the ion density, the standard deviation of ion density variations, and the ion density perturbations (ΔN), respectively.
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