Not only does the Sun try to hide its interior, but it seems to take perverse pleasure in disguising its atmosphere. Van de Hulst's remark, which refers to solar eclipses (that invariably occurred by cloudy weather or after observers have contracted nasty diseases) remains true half a century later, albeit for quite different reasons. And the latter citation reminds us that observation of the outer solar atmosphere is still a difficult art; in opening new windows, progress in techniques has revealed a hierarchy of intricate patterns, reminiscent of a rainforest in which there is a profusion of insects, birds, flowers and trees that we can see but not touch, and whose understanding requires much subtlety.

We took a quick tour of the solar atmosphere in Section 1.2, and we shall now enter into more detail. We will have to complement our plasma physics tool box with some additives, in order to find intellectual coherence in the baroque architecture revealed by observation. By necessity, however, I shall draw an outrageously simplified picture, keeping only a few basic aspects. Far more complete accounts are given for example in [22], [48], [4] and references therein; a lucid survey can be found in [33] for solar activity – of which a nice historical point of view is given in [1].