Sentence examples for electron intensities from inspiring English sources

Using observed quiet-time increases of electron intensities at Earth, we also derive values for this quantity.

The model is used to illustrate how the low-energy electron intensities are affected at different latitudes when enhancing perpendicular diffusion in the polar direction.

Due to the simultaneous registration of the wide range of polar angles in a given azimuth of the sample, measurements of photo- and Auger electron intensities over π steradians can be performed rapidly by azimuthal rotation of the sample.

Figure 5d shows, although there is still the growth bias, as the secondary electron intensities and growth speeds are higher, the possible gap between regions of 1 and 2 is filled, avoiding the neck formation.

We apply the model to compare the simulation results with time series of electron intensities as observed with the SOHO, the IMP 8 and the Ulysses spacecraft and discuss the findings.

This leads to the conclusion that Jovian electron events can unambiguously be observed at heliographic latitudes beyond 40° N. In a Parker-like heliospheric magnetic field, however, there are no field lines connecting Jupiter and Ulysses at >40° N, and therefore, an efficient latitude transport is needed to account for the "high" electron intensities.

Areas with high backscattered electron intensities – light gray levels – represent mineralized matrix with high Ca contents, whereas areas with low intensities – dark gray levels – indicate low mineral density.

In order to derive the dimensions of the gold filaments and of the air holes, we analyzed the secondary electron intensities along a line comprising several Au filaments and air holes.