Solar winds are a result of the sun’s outer atmosphere, known as the corona, being at an extraordinarily high temperature of over a million degrees Celsius. The heat and pressure of the corona propel charged particles away from the sun, and these particles travel at different speeds depending on their source and direction. The slow solar wind has a speed of around 400 km/s, while the fast solar wind can reach speeds of over 800 km/s. Solar winds have a significant impact on space weather, affecting the Earth’s magnetosphere and ionosphere, as well as potentially influencing the evolution of planetary atmospheres throughout the solar system. Understanding solar winds is crucial to predicting and mitigating the effects of space weather.