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A solar prominence extends out from the sun. (Image credit: Mark Johnston)<\/p>\n A solar prominence, also known as a solar filament when seen against the solar disk, is a large bright structure extending from the sun’s surface. The red glowing material is plasma, a hot gas made of charged hydrogen and helium, which flows along twisted magnetic field lines generated by the sun’s internal dynamo<\/a>. When these magnetic structures become unstable, the prominence can erupt, hurling plasma out into space. They are anchored to the sun’s photosphere and extend into its hot upper atmosphere, known as the corona. Prominences can form over about a day and can persist for weeks or even months, looping hundreds of thousands of miles into space, according to NASA<\/a>.<\/p>\n \n Close-up view of the solar prominence as it loops back over the sun. (Image credit: Mark Johnston)<\/p>\n To capture the footage, Johnston used a TEC160FL refractor equipped with a Baader Energy Rejection Filter, Baader 4ZS telecentric, Solar Spectrum 0.3\u00c5 hydrogen-alpha etalon, Lunt hydrogen-alpha etalon, and an ASI174M camera. The result is an astonishing level of detail, revealing the subtle motion of plasma as it interacts with the sun’s dynamic magnetic environment.<\/p>\n <\/p>\n Remember, viewing the sun without the right equipment can be dangerous. Never look directly at it with the naked eye or through a telescope unless you’re using certified solar filters<\/a>.<\/p>\n![\"a](\"https:\/\/www.newsbeep.com\/au\/wp-content\/uploads\/2025\/11\/wmgZRQmxFyMUykPJ72MbiJ.jpg\")
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