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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...

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Bibliographic Details
Main Author: Kyzyurov, Yu.V.
Format: Article
Language:English
Published: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2007
Series:Вопросы атомной науки и техники
Subjects:
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/110409
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