Pela primeira vez, sonda da Nasa observa jato de plasma solar por dentro

É comum o campo magnético do Sol, ejetar jatos de plasma para o espaço.

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São as chamadas - ejeções de massa coronal (CMEs)

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Se uma CME atinge nosso planeta, provoca tempestades geomagnéticas de variadas intensidades.

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Em alguns casos, causam até interrupções de redes elétricas.

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Agora, o instrumento de detecção de luz visível WISPR - Imageador de Campo Amplo da Sonda Solar Parker Solar - registrou redemoinhos no interior do jato.

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Eles indicam a evolução da turbulência durante a interação entre uma CME e o vento solar circundante na área ao redor do Sol.

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Veja agora a imagem captada pelo instrumento:

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