File:Plasmasphere.jpg

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English: This is Image 4 of the NASA article.
These images are taken from a computer animation illustrating the Earth's space storm shield in action. The solar wind, a thin, high-velocity electrified gas, or plasma, blows constantly from the Sun at an average speed of 250 miles per second (400 kilometers/sec). It is represented in Image 1 as a stream of yellow particles flowing from the Sun. The solar wind impacts the Earth's magnetic field, represented by the blue lines in Image 2. As the solar wind flows past the Earth's magnetic field, it generates enormous electric currents that heat Earth's space storm shield -- a layer in the Earth's electrically charged outer atmosphere (ionosphere) -- causing the shield to eject electrically charged oxygen atoms (oxygen ions) into space. The expelled oxygen ions are represented by the green particle streams in Image 3. The ejected oxygen ions gain tremendous speed as they leave the atmosphere, become trapped by the Earth's magnetic field and ultimately encircle the Earth, where they form a billion-degree plasma cloud around the planet, represented by the red cloud in Image 4. The blue doughnut shape in Image 4 represents the high-speed flow of these particles around the Earth. The red "ring of fire" around the Earth's polar regions represents the contribution of the particles to the aurora (the northern and southern lights).
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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Datum a časNáhledRozměryUživatelKomentář
současná15. 6. 2009, 17:24Náhled verze z 15. 6. 2009, 17:241 024 × 768 (91 KB)Sebman81 (diskuse | příspěvky){{Information |Description={{en|1=This is Image 4 of the NASA article. ------------------------------------ These images are taken from a computer animation illustrating the Earth's space storm shield in action. The solar wind, a thin, high-velocity elect

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