Radial distributions of magnetic field strength in the solar corona as derived from data on fast halo CMEs
In recent years, information about the distance between the body of rapid coronal mass ejection (CME) and the associated shock wave has been used to measure the magnetic field in the solar corona. In all cases, this technique allows us to find coronal magnetic field radial profiles B(R) applied to t...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
INFRA-M
2018-03-01
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| Series: | Solar-Terrestrial Physics |
| Subjects: | |
| Online Access: | https://naukaru.ru/ru/nauka/article/20502/view |