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太陽風

17 件の記事

Evolution of PSP design

パーカー・ソーラー・プローブ太陽の深淵に挑む人類史上最速の探査機

パーカー・ソーラー・プローブNASA太陽探査コロナ
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Artist's impression of solar wind flow around Earth's magnetosphere

太陽風の正体と宇宙への影響太陽から吹き出すプラズマの嵐

太陽風コロナプラズマ磁気圏
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The atmospheric gases around Earth scatter blue light (shorter wavelengths) more than light toward the red end (longer wavelengths) of the visible spectrum; thus, a blue glow over the horizon is seen when observing Earth from outer space. The Moon is visible in the background.

惑星大気のメカニズム組成から構造、宇宙への散逸まで

惑星大気天文学大気組成外惑星
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The top image shows the formation mechanism of a normal proton aurora while the bottom image shows the formation mechanism of a patchy aurora.

火星のオーロラ地球とは異なる発生メカニズムと観測の歴史

火星オーロラ磁場MAVEN
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Earth's night-side upper atmosphere appears from the bottom as bands of afterglow illuminating the troposphere in orange with silhouettes of clouds at the top, and the stratosphere in white and blue at the top of the middle. Next, the mesosphere (pink area) extends to the orange and faintly green line of the lowest airglow, at about one hundred kilometres at the edge of space and the lower edge of the thermosphere (invisible). Continuing with green and red bands of auroras stretching over several hundred kilometres.

オーロラの科学夜空を彩る光の正体と宇宙のメカニズム

オーロラ北極光南極光太陽風
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