Two large solar prominences in extreme ultraviolet light (ionized helium at 304) roughly the same size but quite different in structure appeared on the Sun on 18 March 2003. The observation of two large prominences in one image makes this one of the most spectacular images that SOHO has captured. Prominences are large clouds of relatively cool, dense plasma suspended in the Suns hot, tenuous corona. Magnetic fields built up enormous forces that propelled particles out beyond the Suns surface. The one on the right and possibly both were associated with a flare and a coronal mass ejection that blasted away from the Sun at about the time of this image. The twisting nature of the one on the right is of particular interest to some solar physicists who believe that eruptive events like this are the Suns way of getting rid of magnetic fields that are twisted up too tightly, like the rubber bands that run model airplanes

Two large solar prominences in extreme ultraviolet light (ionized helium at 304) roughly the same size but quite different in structure appeared on the Sun on 18 March 2003. The observation of two large prominences in one image makes this one of the most spectacular images that SOHO has captured. Prominences are large clouds of relatively cool, dense plasma suspended in the Suns hot, tenuous corona. Magnetic fields built up enormous forces that propelled particles out beyond the Suns surface. The one on the right and possibly both were associated with a flare and a coronal mass ejection that blasted away from the Sun at about the time of this image. The twisting nature of the one on the right is of particular interest to some solar physicists who believe that eruptive events like this are the Suns way of getting rid of magnetic fields that are twisted up too tightly, like the rubber bands that run model airplanes
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of Two large solar prominences in extreme ultraviolet light (ionized helium at 304) roughly the same size but quite different in structure appeared on the Sun on 18 March 2003. The observation of two large prominences in one image makes this one of the most spectacular images that SOHO has captured. Prominences are large clouds of relatively cool, dense plasma suspended in the Suns hot, tenuous corona. Magnetic fields built up enormous forces that propelled particles out beyond the Suns surface. The one on the right and possibly both were associated with a flare and a coronal mass ejection that blasted away from the Sun at about the time of this image. The twisting nature of the one on the right is of particular interest to some solar physicists who believe that eruptive events like this are the Suns way of getting rid of magnetic fields that are twisted up too tightly, like the rubber bands that run model airplanes by World History Archive/Image Asset Management is available for licensing today.
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Image Number: 1746-19663913Rights ManagedCredit Line:World History Archive/Image Asset Management/SuperStockCollection:Image Asset ManagementContributor:World History ArchiveModel Release:NoProperty Release:NoResolution:4400×4268
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