File:Solar Storm on August 1, 2010.ogv

原始文件(Ogg Theora视频文件,长度19秒,1,280 × 720像素,4.84 Mbps,文件大小:11.1 MB)


摘要

描述
English: The coronal mass ejection starts at 2:36 UTC and ends at 3:56 UTC on August 1 in this animation on STEREO Ahead images. The coronal mass ejection happens quickly. It is the eruption of particles bursting from the left side of the Sun, just below the centre. The animation shows the cloud of particles moving away toward Earth at more than 1,000 kilometres per second (3.6 million kilometres per hour), moving more quickly than any other coronal mass ejection in years.
Македонски: Анимација на исфрлањето на маса од сончевата корона (од 2:36 ч. UTC до 3:56 ч. UTC) на 1 август 2010 г. Облакот од честички се движи кон Земјата со брзина од над 1.000 км/сек (3,6 милиони км/ч).
日期
来源 NASA Earth Observatory
作者 STEREO
其他版本
今日影音 本文件当选为2010年8月16日的今日影音。其说明如下:
English: The coronal mass ejection starts at 2:36 UTC and ends at 3:56 UTC on August 1 in this animation on STEREO Ahead images. The animation shows the cloud of particles moving away toward Earth at more than 1,000 kilometres per second (3.6 million kilometres per hour), moving more quickly than any other coronal mass ejection in years.
其他语言
English: The coronal mass ejection starts at 2:36 UTC and ends at 3:56 UTC on August 1 in this animation on STEREO Ahead images. The animation shows the cloud of particles moving away toward Earth at more than 1,000 kilometres per second (3.6 million kilometres per hour), moving more quickly than any other coronal mass ejection in years.
Македонски: Анимација на исфрлањето на маса од сончевата корона (од 2:36 ч. UTC до 3:56 ч. UTC) на 1 август 2010 г. Облакот од честички се движи кон Земјата со брзина од над 1.000 км/сек (3,6 милиони км/ч).

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Public domain 本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zhNASA版权方针页面JPL图片使用方针。)
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当前2010年8月7日 (六) 13:5519秒, 1,280 × 720(11.1 MB)Originalwana{{Information |Description={{en|1=The coronal mass ejection starts at 2:36 UTC and ends at 3:56 UTC on August 1 in this animation on STEREO Ahead images. The coronal mass ejection happens quickly. It is the eruption of particles bursting from the left si

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