A solar wind is a stream of charged particles (i.e., a plasma) which are ejected from the upper atmosphere of a star.
When originating from stars other than the Earth's Sun, it is sometimes called a stellar wind..
For more information about the topic Solar wind, read the full article at Wikipedia.org, or see the following related articles:
Van Allen radiation belt — The Van Allen radiation belt is a torus of energetic charged particles (i.e. a plasma) around Earth, trapped by Earth's magnetic field. When the ... >
read more
Solar flare — A solar flare is a violent explosion in the Sun's atmosphere with an energy equivalent to tens of millions of hydrogen bombs. Solar flares take place ... >
read more Supergiant — Supergiants are the most massive stars. Supergiants can have masses from 10 to 70 solar masses and brightness from 30,000 up to hundreds of thousands ... >
read more
Solar radiation — Solar radiation is radiant energy emitted by the sun, particularly electromagnetic energy. About half of the radiation is in the visible short-wave ... >
read more
Post a Comment