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\@writefile{lof}{\contentsline {figure}{\numberline {1.2}{\ignorespaces High resolution image of the ``surface'' (photosphere) of the Sun with a resolution of $\sim 140$ km. Granules are seen all around the photosphere outside the dark areas. They form the uppermost layers of the convection zone, in which the energy is transported from deep down outwards via gas motions. At the top, the gas cools down by radiating photons into space. Localized strong magnetic fields can also emerge and are seen as dark areas, the sunspots, which are a consequence of the less efficient energy transport.}}{11}{figure.1.2}}
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