What you will learn

The sun, a G-type main-sequence star, is the center of our solar system and produces a solar wind that creates the heliosphere, a protective bubble that shields us from galactic cosmic rays. However, solar flares and coronal mass ejections can disrupt satellites, communication systems, and power grids, causing significant damage to terrestrial infrastructure. Understanding the sun's behavior and its impact on space is crucial for protecting our technological systems and ensuring their resilience in the face of solar storms.


 

Course curriculum

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About this course

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