[:ja]クリスティーナ・コック宇宙飛行士がISSから撮影したオーロラです。
All in a @Space_Station night. Orbiting at 250 miles up, our nights may only last a half hour, but their beauty will stay with me forever. pic.twitter.com/r4HdRkcA66
— Christina H Koch (@Astro_Christina) December 6, 2019
オーロラは、天体の極域近辺に見られる大気の発光現象です。発生原理は、太陽風のプラズマが地球の磁力線に沿って高速で降下し大気の酸素原子や窒素原子を励起することによって発光すると考えられています。光(可視光)以外にも各種電磁波や電流と磁場、熱などが出ますが、音(可聴音)を発しているかどうかには議論があります。両極点の近傍ではむしろ見られず、オーロラ帯という楕円上の地域で見られやすいです。
参考文献: Christina Koch’s Tweet
地球俯瞰画像を見る: LiVEARTH
[Earthview Wonders][Video] No.1178: Aurora
Astronaut Christina Koch captured from ISS aurora or the northern lights.
All in a @Space_Station night. Orbiting at 250 miles up, our nights may only last a half hour, but their beauty will stay with me forever. pic.twitter.com/r4HdRkcA66
— Christina H Koch (@Astro_Christina) December 6, 2019
An aurora, referred to as polar lights, northern lights, and southern lights, is a natural light display in the Earth’s sky, predominantly seen in the high-latitude regions (around the Arctic and Antarctic). Auroras are the result of disturbances in the magnetosphere caused by solar wind. These disturbances are regularly strong enough to alter the trajectories of charged particles in both solar wind and magnetospheric plasma. These particles, mainly electrons and protons, precipitate into the upper atmosphere (thermosphere/exosphere). The resulting ionization and excitation of atmospheric constituents emits light of varying color and complexity.
Reference: Christina Koch ‘s Tweet
See earthview photo gallery: LiVEARTH[:en][Earthview Wonders][Video] No.1178: Aurora
Astronaut Christina Koch captured from ISS aurora or the northern lights.
All in a @Space_Station night. Orbiting at 250 miles up, our nights may only last a half hour, but their beauty will stay with me forever. pic.twitter.com/r4HdRkcA66
— Christina H Koch (@Astro_Christina) December 6, 2019
An aurora, referred to as polar lights, northern lights, and southern lights, is a natural light display in the Earth’s sky, predominantly seen in the high-latitude regions (around the Arctic and Antarctic). Auroras are the result of disturbances in the magnetosphere caused by solar wind. These disturbances are regularly strong enough to alter the trajectories of charged particles in both solar wind and magnetospheric plasma. These particles, mainly electrons and protons, precipitate into the upper atmosphere (thermosphere/exosphere). The resulting ionization and excitation of atmospheric constituents emits light of varying color and complexity.
Reference: Christina Koch ‘s Tweet
See earthview photo gallery: LiVEARTH[:]