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The SOHO Solar Observatory, managed by NASA and the European Space Agency (ESA), observed the moment when high-energy materials emitted by the sun's surface were emitted earlier this week.
This phenomenon, called "coronal mbad ejection", occurs when the sun releases plasma and the magnetic field from the upper atmosphere.
Coronal mbad releases are a relatively common phenomenon in space weather, but that does not make them observable either: they can send billions of tons of material in space towards our planet, sometimes affecting satellites and communications.
"All the scientific data gathered from the first and second approaches to the Sun have reached the Earth," said Nikalaus Pinkin, head of operations at the Parker Solar Prob mission at APL. Information provided by the spatial probe tools. "
This additional data contains unprecedented visions of the sun, including information on particles, waves, sunflower spray observations and the solar environment.
The Parker Solar probe has been able to withstand some of the most challenging conditions, such as cosmic radiation and hot temperatures.
Due to the mbadive gravity of the sun, the probe has moved faster than any other man made object, flying around the star at 343,000 km / h.
Scientists hope that the revolutionary probe will help solve the mysteries of the sun, such as the warming of the crown (the outer part of the sun's atmosphere) and the way the sun produces huge columns of plasma called solar flares.
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