Figure 1.
Key features of the solar-terrestrial interaction. The solar wind is a constant stream composed of protons, electrons and alpha particles, and its interaction with Earth’s magnetic field shapes the magnetosphere. The region where solar wind pressure is balanced by the geomagnetic field is the magnetopause. Image credit: ESA/NASA - SOHO/LASCO/EIT.

Key features of the solar-terrestrial interaction. The solar wind is a constant stream composed of protons, electrons and alpha particles, and its interaction with Earth’s magnetic field shapes the magnetosphere. The region where solar wind pressure is balanced by the geomagnetic field is the magnetopause. Image credit: ESA/NASA - SOHO/LASCO/EIT.

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