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The rotation of the sun can be monitored by tracking sunspots, magnetic storms on the sun that appear dark against the otherwise bright solar disk. Figure 8.12a shows the initial positions of five spots and fig.8-12b the positions of these same spots one solar rotation later. What can we conclude about the physical nature of the sun from these observations?
Dear Salman There is no figure attached plaese check and re attach the image. I will be happy to help you
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