太陽の表面で発見された巨大コンベクション細胞
David H Hathaway1, Lisa Upton, Owen Colegrove
1NASA Marshall Space Flight Center, Huntsville, AL 35812, USA.
まとめ
巨大な細胞の流れが太陽の内部に流れています.
科学分野:
- 太陽物理 太陽物理学
- ヘリオシズモロジー (ヘリオシズモロジー) とは
- プラズマ物理学のプラズマ物理学
背景:
- コンベクティブ運動は太陽の外層に熱を運ぶ.
- 粒や超粒子は,太陽のコンベクションの表面表現である.
- より大きなコンベクティブ細胞の証拠は,数十年にわたって求められてきました.
研究 の 目的:
- 太陽の巨大な細胞の流れの存在と特徴を調査する.
- 太陽動力学と角運動量輸送におけるこれらの流れの役割を理解する.
主な方法:
- 太陽超粒子の動きを長期間にわたって追跡する.
- 観察データを分析して,継続的な流れパターンを特定する.
主要な成果:
- 何ヶ月も続く巨大な細胞の流れの証拠が見つかりました.
- 観測された流れは,回転によって誘発された方向性を示す (北では時計向き,南では時計逆).
- これらの流れは,太陽の赤道に向かって角運動量を運ぶ.
結論:
- 巨大な細胞の流れは,太陽のコンベクションの重要な特徴です.
- これらの流れは,太陽の急速な赤道回転を維持する上で重要な役割を果たします.
- この発見は,理論的な予測と,大規模な太陽力学に関する観測的証拠を一致させています.
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