ジュピターの強力なオーロラにおける離散的およびブロードバンドの電子加速
B H Mauk1, D K Haggerty1, C Paranicas1
1The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA.
Nature
|September 8, 2017
まとめ
木星
科学分野:
- 宇宙物理学
- 惑星科学
- プラズマ物理学
背景:
- 地球の極光は磁場に沿った電子の加速によって導かれます
- 木星の強烈なオーロラは 類似した離散的なプロセスによって生成されると考えられていた.
- 木星のオーロラに関する以前の観測は 電子の離散加速の証拠を欠いていた.
研究 の 目的:
- 木星の激しいオーロラ放射の 背後にあるメカニズムを調査するために
- 電子加速が木星で起こるかどうかを判断する.
- 木星と地球のオーロラ加速過程を比較する.
主な方法:
- 木星のオーロラ領域のインサイト測定
- 高エネルギー電子加速の分析
- 磁場に合わせた電位を推論する.
主要な成果:
- 木星の極地で 高いエネルギーで 電子の加速を観測した.
- 地球よりはるかに大きい 400キロ電子ボルトまで
- 木星でのブロードバンド/ストキャスティックプロセスよりも エネルギーフローが少ないことがわかりました.
結論:
- 主要なオーロラの原動力ではないのです オーロラの原動力ではないのです
- 木星のオーロラのエネルギー伝達メカニズムは 地球のものと大きく異なります
- 木星上の上向きの電位は 地球上で観測される電位よりもかなり強い.
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