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Updated: Jul 13, 2026

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Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite
Published on: March 11, 2020
太陽のトルション振動のヘリオ・シズミック測定
S V Vorontsov1, J Christensen-Dalsgaard, J Schou
1Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK.
まとめ
太陽のトルション振動は,コンベクティブエンベロープ全体を巻き込みます. これらの表面の回転帯は11年間の太陽周期とともに移動し,内相は極方へ,中緯度から赤道へ広がる.
科学分野:
- ヘリオフィジックスと太陽物理学の研究.
- 太陽の内部動力学と自転に関する研究.
背景:
- 扭転振動,すなわち太陽の回転が変化する帯状は,太陽の表面で観測される.
- これらの振動は,太陽の11年周期を通して緯度に沿って移動します.
研究 の 目的:
- 太陽の内部回転の時間的な変動を調査するために.
- 太陽のコンベクティブエンベロープ内のトルション振動の範囲と動作を決定する.
主な方法:
- 太陽のpモード周波数の分析.
- 太陽とヘリオスフィアの天文台 (SOHO) 衛星のMichelson Doppler Imager (MDI) 装置を使用して約6年間にわたって収集されたデータ.
主要な成果:
- ソーラー・コンベクティブ・エンベロープ全体は,トルション振動に巻き込まれています.
- 内部回転の変動は,中緯度から極方向と赤道方向の両方で相伝播を示しています.
- これらのパターンは,コンベクティブエンベロープ内のあらゆる深さで持続します.
結論:
- 扭転振動は,表面に限定されるのではなく,太陽のコンベクティブエンベロープ全体に広がる現象です.
- 観測された内部相伝播は,太陽のサイクルを駆動するダイナミクスに関する新しい洞察を提供します.
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