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Sunspots: Magnetic Depressions
<< Yesterday 21.03.1998 Tomorrow >>
Sunspots: Magnetic Depressions
Credit & Copyright: National Solar Observatory
Explanation: Our Sun has spots! These spots appear dark in photographs like the one above, but in fact sunspots are quite bright - they are just dark compared to the rest of the Sun. Sunspots are about the size of the Earth and frequently occur in groups, as shown above. Sunspots occur when a concentrated portion of the Solar magnetic field pokes through the surface. This field slows energy from entering the sunspot region, causing sunspots to appear cooler, darker, and lower than the surrounding surface. Sunspots typically last a few days before dissipating. The number of sunspots is always changing, generally going from a maximum to a minimum about every 5 ½ years. In fact, the Sun just passed a minimum two years ago. The Sun and sunspots should never be looked at directly.

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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 - sunspot - Solnechnye pyatna - magnitnoe pole Solnca - Solnechnaya aktivnost' - Solnce
Publikacii so slovami: Sun - sunspot - Solnechnye pyatna - magnitnoe pole Solnca - Solnechnaya aktivnost' - Solnce
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