Figure 7
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Heatmap of the FastDTW alignments between Helio1D (vertical axis) and OMNI (horizontal axis) sequences for (a) solar wind speed, (b) number density, and (c) temperature produced using all the data. Brighter regions have higher probability density than darker regions. Red solid lines show best linear fits with intercepts at zero. Grey solid lines show the lines with slope equal to one.
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