Recently, astronomers unveiled stunning high-resolution images of the sun using a new camera system at the Vacuum Tower Telescope (VTT) in Tenerife. This advanced technology captures intricate details in solar active regions, helping scientists understand solar activity better.
Large sunspot groups often appear during the sun’s activity cycle. With the VTT, researchers can now obtain images that reveal these small structures in remarkable detail. This research was published in Solar Physics.
Typically, large telescopes can zoom in on details but only cover a small area. On the other hand, smaller telescopes provide a broader view but lack fine detail. The VTT strikes a balance by offering both a wide field of view and high spatial resolution, filling a critical gap in solar observation.
With the new camera, researchers can now restore the entire field of view for the first time. This process combines 100 short-exposure images taken at 25 frames per second, producing an 8K resolution image. This technique helps filter out the blurring effects caused by the Earth’s atmosphere.
Rolf Schlichenmaier, a scientist at the Institute for Solar Physics (KIS), emphasizes that understanding solar activity requires studying both the fine structures and long-term developments within active regions. The VTT’s advancements allow for better observation of plasma motions and sunspot groups, which are crucial for understanding solar flares and space weather.
In real terms, the new images cover an area that is a seventh of the sun’s diameter, allowing for the observation of structures as large as 200,000 kilometers. In contrast, many large telescopes cover around 75,000 kilometers. This expanded view is essential for tracking dynamic solar activities.
Robert Kamlah, who worked on the project, shared that their expectations were not only met but exceeded. The findings revealed how sunspots are grounded in larger convective patterns called supergranulation. Scientists utilized specialized filters to spotlight the smallest magnetic field signatures in these solar images.
Looking ahead, the incorporation of low-cost CMOS technologies with 8K resolution could revolutionize solar imaging for future telescopes, offering three times the field of view of current systems.
This new technology not only exemplifies how older telescopes can be enhanced but also proves vital for predicting space weather—information that can significantly impact satellite operations, communications, and even power grids on Earth.
For more in-depth information about this research, refer to Robert Kamlah et al.’s study in Solar Physics (2025) [DOI: 10.1007/s11207-025-02472-6].
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