They are intercepted by Earth's magnetic field.
I calculate about four days. The "slow" solar wind which is the bulk of it, travels at about 400 km/s. The sun is about 149,000,000 km from earth, which works out to about 104 hours. A coronal mass ejection, a massive burst of solar wind with consequences for radio and satellites, may reach earth 1-5 days after eruption.
Solar winds can travel at speeds ranging from 250 to 800 kilometers per second when they reach Earth's vicinity. These high-speed particles are emitted from the Sun's corona and can affect Earth's magnetic field and atmosphere.
The Earth's magnetic field acts as a protective shield against solar winds. This magnetic field deflects charged particles from the sun, preventing them from stripping away the Earth's atmosphere. Additionally, the Earth's atmosphere also helps absorb and scatter some of the energy from solar winds.
Solar Winds
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The magnetosphere serves as a protective shield around Earth, deflecting and trapping most of the solar wind particles. This interaction creates phenomena like the auroras by redirecting charged particles from the solar wind towards the poles. Without the magnetosphere, solar winds would strip away Earth's atmosphere and water.
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Electrical devices such as satellites, power grids, and communication systems can be disrupted by major solar winds hitting Earth. These solar winds can cause geomagnetic storms that lead to disturbances in the Earth's magnetic field, resulting in adverse effects on electronic equipment.
The Earth's two forms of protection against solar winds are its magnetosphere and its atmosphere. The magnetosphere is a magnetic field that deflects most of the solar wind particles, while the atmosphere absorbs and protects the Earth's surface from harmful solar radiation.
Planetary winds are any winds that occur because of solar radiation. They are in direct correlation to the rotation of the earth. Planetary winds do not blow directly north or south.