Magnetospheric response on impact of solar wind diamagnetic structures borne by eruptive prominence
We address the sequence of Sun-to-Earth phenomena, that enables to study the mechanism for geoefficiency of eruptive prominences propagating from the Sun inside coronal mass ejections (CMEs). An eruptive prominence ejected in the solar wind (SW) moves at the SW velocity Earthward like adiamagnetic s...
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| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Mongolian Academy of Sciences
2024-10-01
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| Series: | Proceedings of the Mongolian Academy of Sciences |
| Subjects: | |
| Online Access: | https://www.mongoliajol.info/index.php/PMAS/article/view/3648 |
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