Research news on Solar telescopes

Solar telescopes as a research area encompasses the design, optimization, and scientific exploitation of instruments dedicated to high-resolution, multi-wavelength observation of the Sun. This field integrates optical engineering, adaptive optics, polarimetry, spectroscopy, and imaging techniques to measure solar photospheric, chromospheric, and coronal structures and dynamics. Research focuses on improving spatial, temporal, and spectral resolution; mitigating atmospheric seeing; and extending observations from radio to gamma-ray regimes, including space-based and ground-based platforms. It supports quantitative studies of solar magnetism, flares, coronal mass ejections, and irradiance variability, providing critical data for heliophysics, plasma astrophysics, and space weather forecasting.

Observing oscillations, flares and tornados on the sun

For six and a half days in July 2024, the balloon-borne solar observatory Sunrise III kept its gaze fixed on the sun. The stratospheric flight, which stretched from the northernmost tip of Sweden to Canada's Northwest Territories, ...

Scientists map hidden magnetism on the sun's far side

For observers on Earth, the sun appears as a bright, familiar disk—but what we see is only half the story. Like the moon, one half of the sun is permanently hidden from our direct view: the far side beyond the visible solar ...

Scientists spot a solar flare with surprising spectral behavior

On August 19, 2022, solar astronomers using the Daniel K. Inouye Solar Telescope (DKIST) on the Hawaiian island of Maui caught the fading remnants of a C-class solar flare. Their observations showed something unusual: very ...

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