Solar Cycle: Difference between revisions
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[[ | = Solar Cycle = | ||
== Summary == | |||
The '''Solar Cycle''' refers to the periodic changes in the Sun's activity and appearance, such as variations in the number of [[sunspots]], solar radiation, and solar magnetic field. This cycle, which lasts about 11 years, has significant effects on [[space weather]], Earth’s climate, and [[telecommunications]]. | |||
* [[Solar Cycle 24]] | * [[Solar Cycle 24]] | ||
| Line 5: | Line 7: | ||
* [[Solar Cycle 26]] | * [[Solar Cycle 26]] | ||
[[Precession of the Equinox]] | == What, When, How, Why == | ||
'''What:''' The Solar Cycle is a natural cycle of solar activity, driven by the Sun’s magnetic field, manifesting through changes in the number of [[sunspots]] and solar emissions. | |||
'''When:''' The Solar Cycle averages 11 years, with each cycle starting when solar activity is at a minimum and ending when it reaches the next minimum. | |||
'''How:''' The cycle is primarily caused by the Sun’s magnetic field flipping every 11 years, resulting in a complete 22-year magnetic cycle known as the [[Hale Cycle]]. | |||
'''Why:''' Understanding the Solar Cycle is crucial for predicting [[space weather]], which can impact [[satellite communications]], [[GPS systems]], and [[power grids]] on Earth. | |||
== [[Sun]] - [[Star]] - [[Sol]] == | |||
The Sun, often referred to as '''Sol''', is the star at the center of the [[Solar System]]. Its activity follows the Solar Cycle, which plays a crucial role in the dynamics of the [[Solar System]]. | |||
* The Sun's magnetic activity influences the entire [[Heliosphere]], the bubble of space dominated by the solar wind and magnetic field. | |||
* Increased solar activity during a [[solar maximum]] can lead to intense [[solar flares]] and [[coronal mass ejections]] (CMEs). | |||
For more details, see [NASA - Solar Cycle|https://www.nasa.gov/mission_pages/sunearth/spaceweather/index.html]. | |||
== The Precession of the Equinox == | |||
The '''Precession of the Equinoxes''' is the gradual shift in the orientation of Earth's axis of rotation, which also influences the timing and intensity of solar cycles over millennia. | |||
* This precession impacts the [[Milankovitch Cycles]], long-term changes in Earth’s orbit that affect climate. | |||
* It also has a relationship with the [[Great Year]], the period it takes for one complete cycle of equinox precession. | |||
The [[Precession of the Equinox]] page covers the broader impacts of this phenomenon. | |||
== See Also == | |||
* [[Sunspot Cycle]] | |||
* [[Heliosphere]] | |||
* [[Milankovitch Cycles]] | |||
* [[Space Weather]] | |||
== External Links == | |||
* [NASA - Solar Cycle Overview|https://www.nasa.gov/mission_pages/sunearth/spaceweather/index.html] | |||
* [Space.com - What is the Solar Cycle?|https://www.space.com/solar-cycle.html] | |||
* [NOAA - Solar Cycle and Space Weather|https://www.swpc.noaa.gov/phenomena/solar-cycle] | |||
Latest revision as of 11:46, 15 August 2024
Solar Cycle[edit | edit source]
Summary[edit | edit source]
The Solar Cycle refers to the periodic changes in the Sun's activity and appearance, such as variations in the number of sunspots, solar radiation, and solar magnetic field. This cycle, which lasts about 11 years, has significant effects on space weather, Earth’s climate, and telecommunications.
What, When, How, Why[edit | edit source]
What: The Solar Cycle is a natural cycle of solar activity, driven by the Sun’s magnetic field, manifesting through changes in the number of sunspots and solar emissions.
When: The Solar Cycle averages 11 years, with each cycle starting when solar activity is at a minimum and ending when it reaches the next minimum.
How: The cycle is primarily caused by the Sun’s magnetic field flipping every 11 years, resulting in a complete 22-year magnetic cycle known as the Hale Cycle.
Why: Understanding the Solar Cycle is crucial for predicting space weather, which can impact satellite communications, GPS systems, and power grids on Earth.
Sun - Star - Sol[edit | edit source]
The Sun, often referred to as Sol, is the star at the center of the Solar System. Its activity follows the Solar Cycle, which plays a crucial role in the dynamics of the Solar System.
- The Sun's magnetic activity influences the entire Heliosphere, the bubble of space dominated by the solar wind and magnetic field.
- Increased solar activity during a solar maximum can lead to intense solar flares and coronal mass ejections (CMEs).
For more details, see [NASA - Solar Cycle|https://www.nasa.gov/mission_pages/sunearth/spaceweather/index.html].
The Precession of the Equinox[edit | edit source]
The Precession of the Equinoxes is the gradual shift in the orientation of Earth's axis of rotation, which also influences the timing and intensity of solar cycles over millennia.
- This precession impacts the Milankovitch Cycles, long-term changes in Earth’s orbit that affect climate.
- It also has a relationship with the Great Year, the period it takes for one complete cycle of equinox precession.
The Precession of the Equinox page covers the broader impacts of this phenomenon.
See Also[edit | edit source]
External Links[edit | edit source]
- [NASA - Solar Cycle Overview|https://www.nasa.gov/mission_pages/sunearth/spaceweather/index.html]
- [Space.com - What is the Solar Cycle?|https://www.space.com/solar-cycle.html]
- [NOAA - Solar Cycle and Space Weather|https://www.swpc.noaa.gov/phenomena/solar-cycle]
