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  2. Prominences and sunspots are phenomena associated with the Sun's magnetic field12345:
    • Sunspots are cooler areas on the Sun's surface caused by tangled and knotted magnetic fields.
    • Prominences are tendrils of plasma that unfurl from the solar limb into space, sometimes making the Sun look like a hairy ball when viewed through a telescope.
    • Both sunspots and prominences are caused by the Sun's magnetic fields and sudden releases of stored energy.
    • Prominences consist of ionized gas and neutral hydrogen, often associated with sunspot regions.
    • There are two basic types of prominences: quiescent (long-lived) and transient.
    Learn more:
    Our star is a marvelous orb of seething hot gas. It periodically grows sunspots, “cooler” regions where the magnetic field has become tangled and knotted. Tendrils of plasma called prominences unfurl from the solar limb into space, sometimes making the Sun look like a hairy ball when viewed through a telescope.
    skyandtelescope.org/observing/celestial-objects-to …
    The kinks in the sun’s magnetic field that stick out through the surface are what disrupts the convection and makes a relatively cool place that we see as a sunspot. Another interesting thing that can be seen along a magnetic field line that sticks out of the sun is called a solar prominence.
    www.durangoherald.com/articles/sunspots-and-pro…
    Sunspots are comparatively cool areas of the Sun whose surrounding photosphere often erupts with a high energy flow of particles. These eruptions lead to the formation of both solar prominences and solar flares. Both of these phenomena are caused by the magnetic fields of the Sun and sudden releases of stored energy.
    scopethegalaxy.com/solar-prominence-vs-solar-flare/
    A prominence consists of two ‘foot points’ on the photosphere, often but not always associated with sunspot regions. The material in a prominence consists of a plasma of ionized gas and neutral hydrogen. The ionized gas interacts with the local magnetic field while the neutral hydrogen is kinetically coupled to the ions and ‘dragged along’.
    eclipse2017.nasa.gov/solar-prominences
    There are two basic types of prominences: (1) quiescent, or long-lived, and (2) transient. The former are associated with large-scale magnetic fields, marking the boundaries of unipolar magnetic regions or sunspot groups.
    www.britannica.com/place/Sun/Prominences
     
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    Aug 16, 2024 · Sunspots can be seen on the Sun’s photosphere, or visible surface of the Sun. The number of sunspots goes up and down as the Sun goes through its natural 11-year cycle. Scientists use sunspots to help them track …

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