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  • Solar Wind: Understanding Protons and Electrons from the Sun
    Streams of protons and electrons emitted from the Sun produce solar wind.

    Here's a breakdown:

    * Solar wind: A continuous stream of charged particles (mainly protons and electrons) that flow outward from the Sun's upper atmosphere (corona) at high speeds.

    * Protons: Positively charged particles found in the nucleus of an atom.

    * Electrons: Negatively charged particles that orbit the nucleus of an atom.

    Here's how solar wind is formed:

    1. Sun's activity: The Sun's magnetic field lines become tangled and release energy.

    2. Charged particles: This energy creates a powerful burst of charged particles, including protons and electrons.

    3. Flowing outward: These particles are propelled outward at speeds of hundreds of kilometers per second, creating the solar wind.

    Important Note: The solar wind interacts with the Earth's magnetic field, causing phenomena like:

    * Auroras: Stunning displays of light in the sky.

    * Geomagnetic storms: Disruptions to communication and power grids.

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