FIELD: physics.
SUBSTANCE: invention is intended for short-term forecasting of registration for coronal mass ejection (CME) of the sun. The method of short-term forecasting of registration for coronal mass ejection is based on the analysis of time and spectral data of microwave solar radiation in the period preceding the phenomenon of CME, and includes operations due to processes encompassing a significant part of the Sun at the initial stage, with their subsequent localization in the centers of direct CME formation. This is due to the nature of the ongoing physical processes leading to CME events and their reflection in solar microwave radio emission.
EFFECT: increasing the effectiveness of obtaining a reliable prediction about the movement of an already existing coronal mass ejection.
3 dwg
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