まとめ
極地の平流圏の渦が冷たい空気を隔離し,オゾン層の破壊を可能にします. 航空機のデータは,混合を制限する鋭い境界線を明らかにし,それによってオゾンホールのサイズと将来の潜在的な拡大を制御します.
科学分野:
- ストラトスフィアの科学とは
- 大気化学 大気化学
- 極地気象学 極地気象学
背景:
- 北極地域では,春には劇的なオゾン層の減少が起こります.
- 極地層の平流層の雲と極度の低温は,オゾン層の消失に不可欠である.
- ストラトスフィアの冬の極地渦は,オゾン層の劣化のための条件を作り出します.
研究 の 目的:
- 冬の間,極地渦の構造を調査するために.
- 極地渦とオゾン層の枯渇の関係を理解するために.
- 極地オゾンホールの大きさを制限する要因を評価する.
主な方法:
- 最近の航空機のミッションデータの分析.
- 潜在的渦の傾きを検証する.
- 保守的な微量種の濃度の測定.
主要な成果:
- 極地空気の境界には,潜在的渦巻と微生物の鋭い傾きがある.
- これらのグラデーションは,熱と成分が渦の中に混合することを強く阻害します.
- 極地渦の大きさは,オゾン層の破壊の最大面積を制限する.
結論:
- ヴォルテックス内の極地平流層化学の隔離は,ヴォルテックス崩壊まで,広範囲にわたるオゾン層の減少を防ぐ.
- 南極のオゾンホールの大きさは,現在の限界に達していないため,増加する可能性があります.
- 北半球の極地渦はより小さいので,オゾン層の枯渇の理論的最大値が低い.
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