Properties of Magnetic Features from the Analysis of Near-Infrared Spectral Lines
作者： Sami K. Solanki
DOI: 10.1007/978-94-011-1926-9_48
关键词: Physics 、 Computational physics 、 Near-infrared spectroscopy 、 Spectral line
摘要: An overview is given of the structure and physics magnetic features in solar plages, as derived from observations near-infrared lines. First, diagnostic potential lines compared with that visible at 12 μm. Then, results on velocity obtained 1.5 μm are described, discussed theoretical predictions. Finally, past present achievements investigations Zeeman-split summarized.
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