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It should be noted here that the time axis of Figures 9 and 10 refer to the video and do not include the network delays.
The other solar wind parameters such as V SW, B, B Z, V SW ·B, and ε ′·N P are also examined (taken as horizontal axis of Figures 1 and 2, but not shown here), and the decreased geomagnetic activities for the same solar wind conditions are again obtained for all of these parameters for the majority of hours.
Figure 7 e) shows the profiles through the horizontal axis of Figures 7(a), 7(b), and 7(c) and the theoretical curves.
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Note that on the left-hand axis of Figure 3, GCR counts decrease going up the axis in order to show the relationship with temperature, since fewer GCRs hypothetically means fewer clouds, less reflected sunlight, and higher temperatures.
The observed event miss-ratios (shown in axis of Figure 8(b)) always remain below the required event miss-ratios (illustrated in axis of Figure 8(b)).
On the left axis of Figure 3b, the variation of B with QW thickness is plotted, as extracted from fits in Figure 2b.
(c) Mixture partials are generated according to, where varies between zero and one and represents the dominance of source, as represented in the horizontal axis of Figure 5.
The vertical axis of Figure 3 corresponds to the inverse of the periodicity (i.e., 0.1 corresponds to a 10-year periodicity).
The number of stations referred in the horizontal axis of Figure 12 includes both the source and helper stations, but not the destination.
The upper bound used in each experiment for the differential data values are shown in the axis of Figure 9(c).
On the horizontal axis of Figure 2 several clusters of putatively co-regulated genes are evident.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com