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Fakta Badai Matahari, Capai Bumi Kecepatan Jutaan Kilometer
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Badai Matahari dengan Kecepatan Jutaan Kilometer Capai Bumi
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Tähdet ja avaruus: Merkuriuksen suuri rautaydin saattaa olla magnetismin aikaansaannosta
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Suar Matahari Hantam Bumi, Terbesar dalam 4 Tahun - Teknologi Bisnis com
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Chinese Academy of Sciences
The Sun is not as quiet as it seems, and large or small solar activities caused by solar magnetic field occur every moment. Up to now, all measurements related to the solar magnetic field have been polarization measurements.
Based on the principle of the Zeeman effect, the magnetic field strength can be simply obtained by measuring the Zeeman splitting of a magnetic sensitive spectral line. However, this is almost inapplicable for visible light and near-infrared spectral lines.
The Mg I 12.32 and 12.22 μm lines in the mid-infrared are a pair of emission lines that present a great advantage for accurate solar magnetic field measurement due to their long wavelength, making it possible to directly use the Zeeman splitting formula to measure the magnetic field.