Prominence on the Sun - Search
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  1. History

    The first detailed description of a solar prominence was in 14th-century Laurentian Codex, describing the
    Prominences … See more

    Solar prominence - Wikipedia

    • In solar physics, a prominence, sometimes referred to as a filament, is a large plasma and magnetic field structure extending outward from the Sun's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the much brighter photosphere, and extend outwards into the solar corona. While the corona consists of extremely hot plasm… See more

    Classification

    Historically, any feature that was visible extending above the surface of the sun, including solar spicules, coronal loops, and some coronal mass ejections, was considered a solar prominence. Today, due to a better … See more

    Morphology

    Prominences form in magnetic structures known as filament channels where they are thermally shielded from the surrounding corona and supported against gravity. These channels are found in the chromosph… See more

    Formation

    The exact mechanism which leads to the formation of solar prominences is not currently known. Models must be able to explain the formation of the filament channel and its hemisphere-dependent chirality, … See more

    Eruption

    Some prominences are ejected from the Sun in what is known as a prominence eruption. These eruptions can have speeds ranging from 600 km/s to more than 1000 km/s. At least 70% of prominence eruptions are associa… See more

    Further reading

    • Galsgaard, K.; Longbottom, A.W. (1999). "Formation of solar prominences by flux convergence". Astrophysical Journal. 510 (1): 444–459. Bibcode:1999ApJ...510..444G. doi:10.1086/306559.
    • Golub, L.; Pasachoff J.M. (1997)… See more

     
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  3. In solar physics, a prominence, sometimes referred to as a filament, [a] is a large plasma and magnetic field structure extending outward from the Sun 's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the much brighter photosphere, and extend outwards into the solar corona.
    en.wikipedia.org/wiki/Solar_prominence
    en.wikipedia.org/wiki/Solar_prominence
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  7. Solar filaments, aka prominences, arc upwards

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