Titlebook: Eruptions on the Sun; Boris Filippov Book 2024 The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature

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https://doi.org/10.1007/978-3-658-11623-1 controlled by the magnetic field. All present day prominence models are based on one or other magnetic configuration that creates the magnetic skeleton of the prominence. Other conspicuous plasma structures observed in the corona are coronal cavities, coronal streamers, and polar plumes. Their properties are also briefly discussed.

Axillary

https://doi.org/10.1007/978-3-662-11517-6on. The cause of prominence eruptions seems to be in properties of the prominence equilibrium, the possibility of developing instabilities. The structure of the coronal magnetic field not only determines the height of the onset of eruption, but also guides the direction of the motion of eruptive prominences.

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Equilibrium Plasma Structures in the Solar Atmosphere, controlled by the magnetic field. All present day prominence models are based on one or other magnetic configuration that creates the magnetic skeleton of the prominence. Other conspicuous plasma structures observed in the corona are coronal cavities, coronal streamers, and polar plumes. Their properties are also briefly discussed.

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Introduction,gnetic field, which is the source of solar activity. Some manifestations of the solar activity affect the Earth’s environment and cause disturbances in the terrestrial magnetic field, geomagnetic storms. Solar flares and coronal mass ejections are hazardous for satellites, space stations, and astron