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Updated: Jan 6, 2026

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
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ラジオスペクトル画像を用いて木星の雲の中を覗く
Imke de Pater1, R J Sault2, Bryan Butler3
1Department of Astronomy, 501 Campbell Hall, University of California, Berkeley, CA 94720, USA. Faculty of Aerospace Engineering, Delft University of Technology, 2629 HS Delft, Netherlands. SRON Netherlands Institute for Space Research, 3584 CA Utrecht, Netherlands.
まとめ
木星
科学分野:
- 惑星科学
- 大気科学
- ラジオ天文学
背景:
- 雲の下にある木星の大気は ほとんど未探査のままです
- アンモニア (NH3) は木星の上層大気中の主要な不透明性源である.
研究 の 目的:
- 雲の下にある木星の深層の大気層をマッピングする
- これらの未開拓地域の動的活動と構成を調査する.
主な方法:
- ラジオ波長マッピングに Very Large Array (VLA) を利用した.
- 見える雲より約100km下の8バーの深さまで観測した.
主要な成果:
- 気圧が2~3バー以下で 動的に活動する大気を明らかにした.
- 透明な領域 (低アンモニア濃度) を有する放射熱帯が8バー以下で特定された.
- 深いアンモニアガスを 浅い深さまで運ぶ赤道波を観測した.
- 理論上の5マイクロメートルのホットスポットと相関する無線特性.
結論:
- 木星の深層大気は ダイナミックに活発で 放射熱帯や赤道波のような特徴があります
- 無線観測は 雲に覆われた大気圏に ユニークな窓を開くことができます
- この発見は赤道波を5ミクロメートルの熱点と 結びつける理論を裏付けています
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