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A Solar Prominence Erupts
<< Yesterday 24.09.2001 Tomorrow >>
A Solar Prominence Erupts
Credit & Copyright: SOHO - EIT Consortium, ESA, NASA
Explanation: Our Sun is still very active. Last year, our Sun went though Solar Maximum, the time in its 11-year cycle where the most sunspots and explosive activities occur. Sunspots, the Solar Cycle, and solar prominences are all caused by the Sun's changing magnetic field. Pictured above is a solar prominence that erupted on May 15, throwing electrons and ions out into the Solar System. The image was taken in the ultraviolet light emitted by a specific type of ionized helium, a common element on the Sun. Particularly hot areas appear in white, while relatively cool areas appear in red. Our Sun should gradually quiet down until Solar Minimum occurs in 2007.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: Sun - prominence - maksimum solnechnoi aktivnosti - Solnechnaya aktivnost' - Protuberanec - Solnce
Publikacii so slovami: Sun - prominence - maksimum solnechnoi aktivnosti - Solnechnaya aktivnost' - Protuberanec - Solnce
Sm. takzhe:
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