偏光を用いた太陽磁場計測
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概要
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Magnetic fields play a fundamental role in driving various dynamical phenomena of the solar atmosphere, and the precise measurement of photospheric magnetic fields is of vital importance in solar physics research. A measurement of the spectral line polarizations produced by the Zeeman effect provides the most powerful means for investigating solar magnetic fields. The principle of measurements and some aspects of recent observational results are presented.
- プラズマ・核融合学会の論文
- 2002-08-25
著者
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