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Legal theorists disagree about the proper characterisation of many aspects of the schematic account of the interpretive process given in subsections 2.2 and 2.3 above.
Further details containing justification for varying the student characteristic of "prior exposure" to active learning from experiment I to experiment II and how we implemented the sample selection checks on this parameter are given in subsections 5.4, 5.1, and 6.1, respectively.
More details of GASA are given in Subsections Parts 1 and 2 of GASA.
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More details are given in Subsection 2.5.
Further details are given in subsection with the heading Experiment 2 in Section 6.
Further details about this figure are given in subsection with heading Experiment 3 in Section 6.
We run 100 independent simulations of the model given in Subsection 4.1.
In the observations section, a direct comparison between the observed and calculated ionospheric characteristics with their IRI model-predicted values is given in Subsection 3.1.
Early VLF events with an unusually long recovery (given in Subsection 3.3) are very rare and have not been included in Fig. 3.
In the results section, our general results are presented in Section 3, with diurnal stravior of the key ionospheric parameters of equatorial F region over Ibadan given in Subsection 3.1.
Following a derivation similar to that given in subsection 3.4.1, the overall expected end-to-end per packet energy consumption can be shown to be E [ π E ] = 1 G ∑ e ∈ E f e. π e. (43).
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