Un champ magn\u00e9tique, k\u00e9zako ? \ud83e\uddf2<\/p>\n<\/div>\n
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Il s\u2019agit d\u2019un champ de force qui r\u00e9sulte d\u2019un d\u00e9placement de charges (comme le courant \u00e9lectrique). Pour faire plus simple, le champ magn\u00e9tique, c’est l\u2019espace<\/strong>, autour de l\u2019aimant,<\/strong> d\u2019o\u00f9 les forces magn\u00e9tiques peuvent s\u2019exercer sur d\u2019autres aimants<\/strong>. L\u2019intensit\u00e9 d\u2019un champ magn\u00e9tique se mesure en Gauss<\/strong> ou en Tesla<\/strong>. C\u2019est un peu comme une force invisible<\/strong> qui exerce un pouvoir d\u2019attraction<\/strong>. \u2728<\/p>\n\n <\/div>\n <\/section>\n\n\n\nG\u00e9n\u00e9ralement, les \u00e9ruptions solaires sont dues \u00e0 une accumulation d\u2019\u00e9nergie magn\u00e9tique<\/strong>, et apparaissent en fonction du cycle solaire<\/strong>, qui dure en moyenne 11 ans<\/strong>, car le Soleil n\u2019est pas immuable. Pendant plusieurs ann\u00e9es, il peut ne rien se passer sur le Soleil, puis d\u2019un coup, l\u2019activit\u00e9 va s\u2019intensifier. On parle de maximum solaire<\/strong> lorsque l\u2019activit\u00e9 solaire <\/strong>est au summum de son intensit\u00e9<\/strong>. \u26a1<\/p>\n\n\n\n
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Nicolas<\/p>
CentraleSup\u00e9lec<\/p>
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Hugo<\/p>
Insa Lyon<\/p>
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Olivier<\/p>
La Sorbonne<\/p>
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Agathe<\/p>
ENS Lyon<\/p>
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Emilie<\/p>
Sciences Po Lyon<\/p>
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Margot<\/p>
Arts et M\u00e9tiers ParisTech<\/p>
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David<\/p>
EDHEC<\/p>
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Fanny<\/p>
Ponts ParisTech<\/p>
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