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極光による木星の地球上の上層大気温上昇
J O'Donoghue1,2, L Moore3, T Bhakyapaibul3
1Department of Solar System Science, JAXA Institute of Space and Astronautical Science, Sagamihara, Japan. jameso@ac.jaxa.jp.
Nature
|August 5, 2021
まとめ
木星
科学分野:
- 惑星科学
- 大気物理学
- 宇宙物理学
背景:
- 木星の上層大気は予期せぬほど熱いので 極地帯にオーロラエネルギーが集中している.
- オーロラエネルギーは高緯度で閉じ込められ 重力や音波のような 代替熱源の研究を促しています
- 以前の研究では,惑星全体の高解像度データが不足し,木星の気温のグラデーションと 主要な熱源を決定することができなかった.
研究 の 目的:
- 木星の大気圏上の 地球全体の気温の変動を調べるため
- 木星の大気温分布を 決定する熱源を特定する
- オーロラエネルギー再分配の仮説と 下層大気波の加熱を テストするために
主な方法:
- 木星の赤外線スペクトロスコピーは,高空間解像度 (緯度と経度2度) で行われた.
- 観測は極から赤道まで全惑星をカバーしました
- データ分析は,温度グラデーションをマッピングし,大規模な熱構造を特定することに焦点を当てました.
主要な成果:
- 極光地域から赤道に向かって気温が着実に低下することがわかりました.
- オーロラから広がる可能性のある 太陽風の活動が強化された期間に 高温で惑星規模の構造が観察されました
- これらの発見は 過去のモデルに異議を唱え オーロラ活動と 地球全体の気温との関連を示唆しています
結論:
- 木星の上層大気は主にオーロラからのエネルギーの再分配によって加熱されます.
- オーロラエネルギーは 高緯度では完全に閉じ込められず 地球全体の温度に影響します
- この研究は木星の大気中の支配的なエネルギー転送メカニズムに関する重要な観測証拠を提供します.
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