By Nicole Meyer-Vernet
Creation to sun wind for researchers and graduate scholars in atmospheric physics and astrophysics.
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9 Sunspots have a remarkable property: their number varies in a nearly cyclic way, with a period of about 11 years. They generally occur in groups on the solar disc. 8 (right panel) shows a detailed view of such a group,10 where individual spots appear as a dark umbra about 104 km across surrounded by a ﬁlamentary penumbra. Some sunspots may last for weeks; this has enabled early observers to follow their motion and to ﬁnd that the Sun appears to rotate about its axis once in about 27 days (as seen from Earth).
25 Drawing of the appearance of the corona at the 30 June 1954 eclipse, near solar activity minimum. ) dimensions, it forms an annular current sheet that separates the magnetic ﬁelds originating at opposite poles. Although Fig. 24 refers to a highly idealised situation, the real corona might sometimes resemble it, as suggested by Fig. 25, which is an old drawing of the visual appearance of the corona during a solar eclipse . One must be cautious in interpreting such visual appearances since they result from diﬀerent structures lying along the line of sight of the observer, and projection eﬀects can be misleading.
1980, The scientiﬁc objectives of the international solar polar mission, Phil. Trans. Roy. Soc. London A 297 565. -P. 1992, The Ulysses mission, Astron. Astrophys. Suppl. Ser. 92 207.  Zirker, J. B. 2002, Journey from the Center of the Sun, Princeton University Press. 2 Tool kit for space plasma physics Most of the Universe is made of plasma. And yet, plasmas are very rare on the Earth, where solids, liquids and gases – the three primary states of matter – are ubiquitous (Fig. 1). These states are the result of a competition between thermal energy and intermolecular forces.
Basics of the Solar Wind by Nicole Meyer-Vernet