まとめ
バルーンで運ばれるボロメーターを用いた遠赤外線天気調査は,星間粒子の熱放射線を探した. 月だけが検出され,他の天文源の上限を設定しました.
科学分野:
- 天文学と天体物理学について
- コスミック・マイクロ波・バックグラウンド・放射線
背景:
- 星間粒子は,星間媒体の重要な構成要素である.
- 遠赤外線放射は,宇宙の熱過程についての洞察を提供します.
研究 の 目的:
- 恒星間粒子の熱放射線を探すために.
- 空の遠赤外線放射の局所的な源を特定するために.
主な方法:
- 液体ヘリウムで冷却された気球搭載のゲルマニウムボロメーターを使用した.
- 遠赤外線観測のために,スペクトルフィルター付きの望遠鏡を使用しました.
- 北の銀河系を含む天球の約半分をカバーする調査を実施した.
主要な成果:
- 月からの熱放射線のみが検出されました.
- 他の源からの微分流量の上限を2x10{\displaystyle 2x10{\displaystyle 2x10{\displaystyle 2x10{\displaystyle 2x10{\displaystyle 2{\displaystyle 2{\displaystyle 2}) W/cm2/Hzで設定した.
- ブラックボディの発生源に対するシステムの反応は,主に300〜360ミクロンであった.
結論:
- 初期調査では,星間粒または他の局所的な源からの有意な遠赤外線熱放射線は検出されなかった.
- 月は,この機器で検出可能な遠赤外線放射の主要な源です.
- この研究は,将来の淡い宇宙源の探査のための重要な上限を設定しています.
関連する概念動画
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When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
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