隠された彗星の尾の海雪は 海洋による炭素の吸収を妨げています
Rahul Chajwa1, Eliott Flaum1,2, Kay D Bidle3
1Department of Bioengineering, Stanford University, Stanford, CA 94305, USA.
まとめ
海洋の炭素貯蔵に不可欠な 雪の沈み方は 以前は未知だった"彗星の尾"によって 遅くなっています これらの構造は,エクソポリマーハロによって形成され,粒子の滞在時間を延長し,気候の調節に影響を与えます.
科学分野:
- 海洋学
- 生地化学
- 流体力学
背景:
- 海の積雪は 気候を調節する 海洋の生物学的炭素ポンプに不可欠です
- 海の雪の沈着の物理学的理解は,集積の複雑さと直接の観測の欠如によって制限されています.
研究 の 目的:
- 海洋積雪の微水力学と沈殿物理学の調査.
- 沈没のダイナミクスに与える影響を明らかにします
主な方法:
- 野外でのスケールフリー垂直追跡顕微鏡を使用した.
- 堆積物から採取した新鮮な海雪を微水力学的に測定した.
主要な成果:
- エキソポリマーハローによる 彗星のような新形態を発見した
- これらの"彗星の尾"は 粒子の沈没速度を大幅に遅らせます
- これらの構造が水柱に留まる時間を 延ばすことが示されています
結論:
- この研究により,以前は知られていなかった 流体構造の相互作用が 海洋の雪沈没を制御していることが明らかになりました
- これらの粒子のストーケシアン沈着の縮小型モデルが開発された.
- 発見は海洋の生物学的炭素ポンプと 気候の調節に関する 予測的な理解を前進させています
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