Sentence examples for electron intensity from inspiring English sources

When an electron beam intersects the standing light wave at a right angle, it forms a distinctive "bright" and "dark" pattern of electron intensity beyond, heralding electron diffraction.

The results show that the Jovian electron intensity varies by a factor of ∼10 during this cycle of magnetic connectivity.

The dynamics of L-distribution of the relativistic electron intensity is superimposed to the solar wind and magnetosphere variations.

On the contrary, extremely low substorm activity surely observed during whole the storm recovery phase constitutes a sufficient condition of the non-increased after-storm electron intensity.

Positions of both the ring current maximum and electron intensity maximum (Lmax) are consistent to our previous result: |Dst|max = 2.75 104/L4max.

The results show how the relative contribution of low-energy galactic and Jovian electrons vary with respect to the total electron intensity for the various diffusion coefficients.

In particular, the electron intensity-time-profile along the Ulysses trajectory is calculated for various diffusion coefficients and compared to the 3 – 10 MeV electron flux observed by Ulysses.

It is illustrated how the electron intensity-time profile along the Ulysses trajectory is effected as compared to the 3 10 MeV electron flux observed from its launch until the recent solar maximum conditions by varying.

To track the bubble's location throughout the growth process, instead of taking the area centroid, we account for the three-dimensional shape of the bubble by taking the detected electron intensity-weighted centroid, where each pixel is multiplied by its intensity value.

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.