Loading...

Glossary term: 태양활동주기

Description: 태양활동주기는 태양에서 흑점, 태양플레어, 그리고 다른 형태의 활동이 약 11년 주기로 반복되는 현상을 말합니다. 이러한 태양의 활동은 태양 자기장의 변화에 의해 일어납니다. 태양의 자기장은 약 11년마다 방향이 바뀌어, 북극과 남극의 자기극이 서로 바뀝니다. 따라서 태양의 자기장이 다시 원래 방향으로 돌아오려면 약 22년이 걸립니다.

Related Terms:



See this term in other languages

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".

If you notice a factual or translation error in this glossary term or definition then please get in touch.

In Other Languages