ilmankierto

Ilmankierto, also known as the annual solar cycle, is a periodic variation in the Sun's activity that occurs approximately every 11 years. This cycle is marked by changes in sunspot number, solar irradiance, and the Earth's magnetic field. During the solar maximum phase, sunspots are most numerous and solar activity is highest. Conversely, during the solar minimum, sunspots are rare and solar activity is lowest.

Sunspots are temporary phenomena on the Sun's surface, appearing as dark spots due to their lower temperature compared to the surrounding areas. The number of sunspots varies over the solar cycle, with a peak in activity around solar maximum and a minimum around solar minimum. This variation is not perfectly periodic and can differ in length and intensity from one cycle to the next.

The solar cycle has significant implications for Earth's climate and space weather. During solar maximum, increased solar activity can lead to more intense solar flares and coronal mass ejections, which can disrupt satellite operations, power grids, and communication systems. Conversely, during solar minimum, there is a reduced risk of these disruptions. The solar cycle also influences the Earth's magnetic field, which can affect the intensity of auroras and the distribution of radiation belts.

The solar cycle is monitored by space-based observatories such as the Solar and Heliospheric Observatory (SOHO) and the Solar Dynamics Observatory (SDO). These missions provide data on sunspot number, solar irradiance, and other solar activity indicators, which are used to predict the phase of the solar cycle and its potential impacts on Earth and space. Understanding the solar cycle is crucial for space weather forecasting, satellite operations, and the development of technologies that can mitigate the effects of solar activity on Earth.