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When fusion reactions occur in a plasma, the power released is proportional to the square of plasma ion density, n2.
The F region has two maxima (i.e., two periods of highest ion density) during daylight hours, called F1 and F2.
Both the F1 and F2 regions possess high ion density and are strongly influenced by both solar activity and time of day.
Of these, the F2 region is the more variable of the two and may reach an ion density as high as 106 electrons per cubic centimetre.
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.
The deep depletions of the ion density are plasma bubbles.
Shown in the bottom row is the ion density.
This is the reason why the ion density is largely less than that of electron, i.e., ion density is seriously underestimated.
With increasing anode current, ion density and electron temperature increased.
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