ЗАКОНОМІРНОСТІ ЕВОЛЮЦІЇ ВЕЛИКОМАСШТАБНИХ МАГНІТНИХ ПОЛІВ НА СОНЦІ ЗА ДАНИМИ СПОСТЕРЕЖЕНЬ
Based on the observational data the evolution over three solar cycles of large-scale solar magnetic fields is studied and the general change pattern of solar cycles of weak photospheric and strong (in active regions) fields is determined. It is found that, along with significant differences in the e...
Збережено в:
| Дата: | 2025 |
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| Автори: | , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
V.M. Glushkov Institute of Cybernetics of NAS of Ukraine
2025
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| Онлайн доступ: | https://jais.net.ua/index.php/files/article/view/603 |
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| Назва журналу: | Problems of Control and Informatics |
Репозитарії
Problems of Control and Informatics| Резюме: | Based on the observational data the evolution over three solar cycles of large-scale solar magnetic fields is studied and the general change pattern of solar cycles of weak photospheric and strong (in active regions) fields is determined. It is found that, along with significant differences in the evolution of weak and strong magnetic fields, there is a close relationship of their behavior in the selected strength intervals, if as characteristic for comparison the growth rate of the total field flux is considered. Currently there are no argued theoretical explanation of the relationship determined in the article, and the problem of its interpretation is the subject of a separate research. |
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