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After this boundary, there were no further instances of the maximum energy flux for the three energy bins with two consecutive values exceeding 1 × 108 eV cm−2 s−1 sr−1 eV−1.
At 08 26 47 UT, the integral number flux ratio increased sharply, and the maximum energy flux of the electron precipitation for the three energy bins around 100 eV no longer reached 1 × 109 eV cm−2 s−1 sr−1 eV−1.
In the electron spectrogram (Figure 4b), this boundary represents the point where the maximum energy flux for the three energy steps around 100 eV first exceeded 1 × 108 eV cm−2 s−1 sr−1 eV−1 (yellow color) for two consecutive seconds.
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It would be preferable to install a wave energy converters in a wave state having a maximum total energy flux rather than in one having maximum occurrence.
It can be observed again that the wave state of maximum occurrence does not coincide with the wave state of maximum total energy flux.
From Fig. 9b, c, it can be observed that the wave state of maximum occurrence does not coincide with the wave state of maximum total energy flux.
For the present event, the maximum differential energy flux at approximately 100 eV similarly exceeded 1 × 109 eV cm−2 s−1 sr−1 eV−1 in both regions.
The maximum electron energy flux from the three energy bins around 100 eV decreased to values below 1 × 108 eV cm−2 similar1 eV−1, similar to the values often observed prior to Boundary 2. In addition, at this time, the energy flux of the ion precipitation sharply increased and approached that observed before Boundary 2. We refer to the region between Boundaries 2 and 3 as Region b.
The sensitivity and the maximum of the measurable energy flux can be influenced by the geometry of the probe holder.
That is why in spite of intense radial diffusion, the L-position of the maximum of phase space density of relativistic electrons coincides with the position of the maximum of the precipitating ion energy flux (ion pressure) and the equatorial boundary of the region of the substorm dipolarizations.
It is possible to see that the maximum of the precipitating ion energy flux (b2i boundary introduced by Newell et al. (1996)) is located near the 60° geomagnetic latitude which corresponds to L = 4, where L is the McIlwain parameter).
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