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A new detailed image of the outer solar body, known as Corona or Aura Sun, reveals that this solar layer is not smooth as previously thought but that it is organized and dynamic.
The Corona layer is very hot and the source of the solar wind, that is, charged particles emanating from the sun. It was difficult to understand how the solar wind had formed with previous images of the crown showing that the sun's surface was relatively polished.
"Previous images showed that the outer corona was a soft structure, but in deep space, the solar wind is turbulent and dusty," said Dr. Craig Davis.
Using new imaging techniques, "the team realized that the Corona layer was not smooth but dynamic," he said.
The team at the Southwest Institute Institute Research Institute used the COR-2 tool from NASA's STEREO-A Observatory to access this discovery and capture the details of the research of the 39, plasma atmosphere of the atmosphere.
Recall that the research team was able to remove the scrambling of the series of images using anatomy algorithms, and adjust the brightness to get the gorgeous scenes.
Source: RT
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