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Glossary term: Cycle solaire

Description: Le cycle solaire est le cycle d'environ 11 ans du nombre de taches solaires, d'éruptions solaires et d'autres formes d'activité sur le Soleil. Cette activité est générée par le champ magnétique global du Soleil. Comme ce champ magnétique passe de la polarité nord à la polarité sud tous les onze ans, il faut une période complète de 22 ans pour que les pôles magnétiques du Soleil retrouvent leur configuration d'origine.

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".