Method to study the “traces” of coronal mass ejections
Scientists at Skolkovo Institute of Science and Technology (skoltech), together with colleagues from the Karl-Franzens University of Graz and the Kanzelhoehe Observatory (Austria), have developed an automatic method for detecting coronal dimmings, or traces of coronal mass ejections from the sun; they have also proved that these are reliable indicators of the early diagnosis of powerful emissions of energy from the atmosphere of the sun traveling to Earth at great speed. The results of the study are published in the Astrophysical Journal.
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