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Image for: First solar observations with unique instrument at the world's largest solar telescope


Fig. 2: Solar atmosphere in the filtergram channel at a wavelength of λ = 588.9 nm. In the darker areas, the solar plasma has lower temperatures than the surroundings which means that the luminous flux is lower. These areas are referred to as sunspots.
Fig. 2: Solar atmosphere in the filtergram channel at a wavelength of λ = 588.9 nm. In the darker areas, the solar plasma has lower temperatures than the surroundings which means that the luminous flux is lower. These areas are referred to as sunspots.

VTF/KIS/NSF/NSO/AURA

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