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Modélisation de l'évolution du réseau magnétique au cours du cycle solaire

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Figure

Figure 1.1: Le Soleil observ´ e en intensit´ e en lumi` ere visible. Les taches y sont apparentes, ainsi que les facules pr` es des bords
Figure 1.2: Un magn´ etogramme solaire. Le champ magn´ etique d´ etect´ e est dans la ligne de vis´ ee
Figure 1.3: Le Soleil vu en coupe. L’axe vertical correspond ` a l’axe de rotation, tandis que l’axe horizontal d´ ecrit le plan ´ equatorial
Figure 1.4: Les cellules de convection de la surface solaire (granules). Il s’agit d’une image en intensit´ e, o` u les r´ egions claires sont plus chaudes et les r´ egions sombres, plus froides
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