Solar Winds


Solar winds are a stream of charged particles, mainly protons and electrons, that are continuously emitted from the upper atmosphere of the Sun. These winds can travel at speeds of up to 900 km/s and can have a significant impact on the space environment, including the Earth's magnetosphere and ionosphere. The study of solar winds is important in space and astronautical engineering as it helps in understanding the effects of space weather on spacecraft and communication systems. It also plays a crucial role in the design and operation of space missions, particularly those that involve interplanetary travel.


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