Sentence examples for mean electron density from inspiring English sources

At higher altitude, δNe is mainly larger than zero, and the March DE3 tide increases the zonal mean electron density.

It is also reported that DE3 tides drive an equatorial ionization anomaly (EIA) structure at higher ionosphere in the relative difference of zonal mean electron density.

At lower altitude (below about 170 km), δNe is mainly less than zero, and the March DE3 tide decreases the zonal mean electron density.

Different programs sometimes produce data with the same label but a different interpretation; does "density" mean electron density or mass density?

The influence of DE3 tide on the equinoctial asymmetry of the zonal mean electron density varies with latitude, altitude, and solar activity level.

The mean electron density varies from 28.4 225 cm −3, which corresponds to the harmonics m = 1 8 at the mean reflection height of 81.5 87.7 km.

The relative difference between two cases is calculated as Figure 2 The altitudinal and latitudinal variations of the simulated zonal mean electron densities.

With the effect of the 'fountain effect', the equatorial ionization anomaly (EIA) appears in the mean electron densities, and the low-latitude ionosphere is higher than the mid- and high-latitude ionospheres.

The bottom plots show the altitudinal and latitudinal variations of the relative difference of the zonal mean electron densities for low solar activity level (c) and for high solar activity level (d).

The altitudinal and latitudinal variations of the simulated zonal mean electron densities at September driven by (a) September DE3 tide (in a unit of 1011/m-3) andrivenen by (b) March DE3 tide (in a unit of 1011/m-3); the relative difference of the zonal mean electron densities between (c) two simulations (δNe) (in a unit of %) and the (d) altitudinal profiles of δNe (in a unit of %).

They have reported mean peak electron density (1.33 ± 0.5) × 104 cm−3 in the meteoric layer at a mean altitude of 91.7 ± 4.8 km.