Spectrum of small-scale plasma structures in the photosphere
In this report we consider possibility of formation of small-scale plasma structures in the turbulent flows of photospheric gas on the Sun and analyse dependence of their spectrum and intensity on height and the magnetic field strength. It was shown that in the height range 150–350 km the slope of t...
Збережено в:
| Дата: | 2007 |
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| Автор: | |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
2007
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| Назва видання: | Вопросы атомной науки и техники |
| Теми: | |
| Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/110409 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | Spectrum of small-scale plasma structures in the photosphere / Yu.V. Kyzyurov // Вопросы атомной науки и техники. — 2007. — № 1. — С. 81-83. — Бібліогр.: 9 назв. — англ. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| Резюме: | In this report we consider possibility of formation of small-scale plasma structures in the turbulent flows of photospheric gas on the Sun and analyse dependence of their spectrum and intensity on height and the magnetic field strength. It was shown that in the height range 150–350 km the slope of the structure spectrum decreases with increasing the altitude. Under the weak magnetic field (B = 5 G), the intensity of plasma structures is unchanged with height. The increase in the magnetic field strength results in a rise in the structure intensity and in a decrease in the spectral slope. |
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