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On Quasi-biennial oscillations in chromospheric macrospicules and their potential relation to global solar magnetic field

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Figure

Figure 1. In the left column in each panel, raw data of the properties of MS are marked with blue dots and their running average is highlighted with red dots with anrepresent the 1errorbar
Figure 2. QBOs in various parameters of solar activity phenomena. The top panel contains three MS properties, which indicate QBOs: maximum length (red solidline), average velocity (blue solid line), and maximum area (green solid line)
Table 1
Figure 3. Cross-correlations between the three MS properties and thedata after 2013 May
+2

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