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Abstract: Main problems of magnetic storm prediction and causes of low efficiency ofmedium-term prognosis are discussed. It is supposed, that possible way of theirsolving is searching for poor-investigated features of solar wind forinstance, solar wind density behavior before storms. The necessity ofinvestigation not only severe storms and coronal mass ejections CMEs, butorigin of moderate and weak storms is shown. Examples of successfulinvestigations in this direction are given.



Autor: Olga Khabarova

Fuente: https://arxiv.org/







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