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| ==== Current year ==== | ==== Current year ==== | ||
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| + | === October 2026 === | ||
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| + | <columns 100% l > | ||
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| + | <img src=" | ||
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| + | The 2026 THEMIS observation season started this month of September with four ~1 week campaigns. With the new magnetic inversion pipeline (based on the UNNOFIT code) of the Fe I @ 630,2 nm spectropolarimetric observations, | ||
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| + | The present image displays a sample of September 2026 maps of the line-of-sight component of the vector magnetic field of different solar structures: quiet sun, filament corridors, plages, inter-spot regions and sunspots. Blue means that the photospheric magnetic field is orientated toward the observer, while red means away. In all these observations, | ||
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| + | These high-spatial and high-spectral resolution observations, | ||
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| === September 2026 === | === September 2026 === | ||