Solar Activity: The Sun's Dynamic Behavior and Its Impact on Earth

On the Sun's surface and in its atmosphere, there are many different kinds of action. Here are some of the most common:

Sunspots: They are dark spots on the surface of the Sun that are caused by the magnetic field of the Sun. they are located at photosphere. Sunspots can be different sizes and shapes, and they usually come in pairs. Why they appear dark? 🙆 Because here temperature is down than their surroundings. Dark central of sunspot is known as umbra and surrounded by less dark region, called penumbra. Why is the temperature of the sunspots lower than their surroundings? 🙆 It is due to the existence of strong magnetic fields in the sunspots.

Solar flares: Solar flares are rapid, powerful bursts of energy that happen on the surface of the Sun and send out a lot of radiation into space. Coronal mass ejections (CMEs) can happen at the same time as solar flares. It happens near to sunspots.

Coronal mass ejections (CMEs): CMEs are big blasts of plasma from the Sun's corona that can move at up to 3 million kilometers per hour. CMEs can change the Earth's magnetic field and atmosphere in big ways. In CMEs, billons of tons of coronal material are released, in which mainly electron, protons, ions, plasma and magnetic field are present. This material spread into far space. And meet with solar wind they travel long distances and affects the planets and satellites.

Prominences: They are big, bright loops of gas that stick out from the surface of the Sun. They are made by the Sun's magnetic field. Prominences can be seen during a sun eclipse and can last for weeks.

Solar wind: Solar wind is a flow of charged particles that comes from the Sun and changes the magnetic field of the Earth. The solar wind can cause the Northern and Southern Lights and can also mess up communications and power lines.

Solar storm: Solar storms are strong releases of energy and charged particles from the Sun's atmosphere. They are also called solar flares or coronal mass ejections (CMEs). Solar storms happen when magnetic energy builds up in the Sun's atmosphere and is quickly released as powerful bursts of radiation and particles. Most of the time, they are linked to sunspots, which are spots on the Sun's surface with strong magnetic fields. When the magnetic fields get twisted and jumbled, they can cause a huge amount of energy to be released all at once.
Geomagnetic storm: A geomagnetic storm is a disturbance in Earth's magnetosphere caused by solar activity.


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