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It is known that long-lasting solar flares like this one are very eruptive. In addition to a type II radio emission, a large amount of plasma was also emitted from the sun, as can be seen in the picture:
You can see a large and fast coronal mass ejection, both on the coronagraph images from SOHO and the images from STEREO A. The speed of this coronal mass ejection is estimated to be around 1,400 km / s which is very fast. Due to the peripheral location of the eruption, the plasma cloud is directed away from the earth and an impact on our planet is not expected.
Our sun is slowly picking up speed, the exciting phase has begun!