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Spicules

Photo of the chromosphere above the active region of the Sun No. 10380 in the line of hydrogen H α . The characteristic texture of the chromosphere, resembling “burning prairies ”, is created by spicules.

Spicules (from lat. Spiculum - tip, tip) - the main elements of the fine structure of the chromosphere of the Sun. If we observe the limb of the Sun in the light of a certain spectral line , then the spicules will be visible as rather thin columns of a luminous plasma on the scale of the Sun (with a diameter from 500 to 1200 km ). These columns are ejected from the lower chromosphere at a speed of about 20 km / s 5-10 thousand km up. Spicula lives 5-10 minutes, its maximum length is from 10 to 20 thousand km . The number of spicules existing on the Sun at the same time is about a million, they cover about 1% of the solar disk. Almost all spicules are on the boundaries of supergranules ; Thus, the chromospheric network consists precisely of them.

Links

  • The mechanism of heating the solar corona may be revised
  • Scientists have discovered the origin of spicules in the sun

Literature

  • Priest E.R. Solar magnetohydrodynamics. - M .: Mir, 1985. - S. 44-48.


Source - https://ru.wikipedia.org/w/index.php?title=Spicules&oldid=100327436


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Clever Geek | 2019