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Maximum electron densities up to 7 × 1011 cm− 3 were obtained during the transient phase.
On the nightside the echoes are often very diffuse and highly irregular, with maximum electron densities less than 104 cm−3.
The maximum electron densities predicted due to ablation of micrometeoroids and meteoroids of velocities 10 km/s and 30 km/s respectively are comparable in magnitude with these measurements.
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A π bond also helps to hold the two atoms together, but, because the region of maximum electron density produced by the overlap is off the line of the internuclear axis, it does not do so with the same strength as a σ bond.
The maximum electron density is about 1.2 × 1018 m-3.
The maximum electron density on the oxygen atom is responsible for the polarity of the molecule.
On the dayside of Mars the maximum electron density is approximately 2 × 105 cm−3.
From the GPS-reconstructed images the quantity assessed was the maximum electron density at the F-layer peak height (Nmax).
Each layer (represented by a portion of the profile) is characterized by the three parameters: local maximum electron density (or maximum plasma frequency), corresponding height, and semi-thickness.
The end product is a set of 114 electron density profiles as functions of radial distance and altitude, each accompanied by orbit number, date, latitude, longitude, solar zenith angle, radius of areoid, radial distance to maximum electron density, altitude of maximum density, and maximum electron density.
The maximum electron density surrounding the plasma depletions in such cases might be close to that of the peak electron density of the unperturbed background ionosphere.
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