惑星大気の記事

マーガレット・A・トルバート極成層圏雲の研究をリードする大気化学者

マーガレット・A・トルバート大気化学極成層圏雲オゾン層破壊

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Figure 1. Carbon dioxide pressure-temperature phase diagram

超臨界流体の特性と産業利用液体と気体の境界を超える物質の状態

超臨界流体臨界点二酸化炭素超臨界水

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A picture of Earth's troposphere with its different cloud types of low to high altitudes casting shadows. Sunlight is reflected off the ocean, after it was filtered into a reddish light by passing through much of the troposphere at sunset. The above lying stratosphere can be seen at the horizon as a band of its characteristic glow of blue scattered sunlight.

対流圏の仕組みと地球環境への影響

対流圏大気構造対流圏界面気温減率

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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.

惑星の大気宇宙のガス層が形成される仕組みと多様な組成

惑星大気天文学大気組成太陽系

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Representation of an organic compound hydroxy group, where R represents a hydrocarbon or other organic moiety, the red and grey spheres represent oxygen and hydrogen atoms respectively, and the rod-like connections between these, covalent bonds.

ヒドロキシ基の化学的性質と宇宙における存在

ヒドロキシ基水酸基化学結合水素結合

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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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