News on the Sun
- The Sun has shifted ppolarity
- Huge tornadoes discovered on the Sun
- The Sun got bigger
- Last solar minimum was unusual
- The sound of a solar storm
- Earth’s magnetic field provides vital protection
- The Sun's magnetosphere
- IBEX detects "alien" particles
- Cold Hydrogen gasses recycles sunspots
- Thin layers of cosmic chok-waves
- The Solar cycles
- Comet hits the Sun
- Solar eruption causes massive Aurora's
- Our Solarsystem had a fifth Gas-giant planet
- 6 Coronal Mass Ejections in 24hours!
- New Characteristics of Solar flares discovered
- 40 year old Mariner 5 solar wind problem solved
- Solar wind traced in 3D from Sun to Earth
- Detection of emerging sunspot regions
- SDO Spots Extra Energy in the Sun's Corona
- New images of Vesta from DAWN
- New way to measure magnetism around the Sun
- Solar eruption "blew half the sun to pieces"
- Sun and planets constructed differently
- Solar storm reaches Earth today
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The Solar cycles
Friday, 28 October 2011 10:57
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| Solar system - The Sun |
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Telescopes has spotted sunspots since 1611. While the sun had long been thought to be an unchanging, "perfect" orb, sky-watchers observed black sunspots on the sun's surface that circled around as with the sun's rotation.
That first crack in the theory of the sun's immutable nature would soon fracture completely as the number of sunspots were shown to increase and decrease over time in a regular, approximately 11-year cycle, called the sunspot cycle. The exact length of the cycle can vary. It has been as short as eight years and as long as fourteen, but the number of sunspots always increases over time, and then returns to low again.
More sunspots mean increased solar activity, when great blooms of radiation known as solar flares or bursts of solar material known as coronal mass ejections (CMEs) shoot off the sun's surface. The highest number of sun spots in any given cycle is designated "solar maximum," while the lowest number is designated "solar minimum." Each cycle varies dramatically in intensity with some solar maxima being so low as to be almost indistinguishable from the preceding minimum.
It was not until the first half of the 20th century that scientists began to understand what causes the sunspot cycle. Researchers determined that the sunspots were a magnetic phenomenon and that, indeed, the entire sun was magnetized with a north and a south magnetic pole just like a bar magnet. The comparison to a simple bar magnet ends there, however, as the sun's interior is constantly on the move. Source: NASA |






