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NSF’s DKIST Captures Sharpest Ever Images of Fine Solar Magnetic Striations

NSF’s DKIST Captures Sharpest-Ever Images of Fine Solar Magnetic Striations

NSF’s DKIST captured ultra-fine magnetic striations on the Sun’s surface, just 20 km wide.

Written by Gadgets 360 Staff | Updated: 18 June 2025 12:33 IST

NSF’s DKIST Captures Sharpest-Ever Images of Fine Solar Magnetic Striations

Photo Credit: NSF/NSO/AURA

DKIST Uncovers Ultra-Thin Magnetic Striations on the Sun’s Surface, Offering New Solar Insights

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Highlights

DKIST reveals 20-km wide magnetic striations on Sun’s granules
Striations trace fine magnetic field variations in solar photosphere
Discovery may improve solar storm and space weather forecasting

In a new study using the NSF's Daniel K. Inouye Solar Telescope (DKIST), scientists captured the sharpest-ever views of the Sun's surface, revealing ultra-narrow bright and dark “striations” only ~20 kilometers wide. These striations – alternating light and dark bands on the walls of solar granules – arise from tiny fluctuations in the magnetic field, tracing the Sun's magnetism. DKIST's unmatched 4-meter mirror achieved ~0.03″ (~20 km) resolution – roughly the length of Manhattan Island – unveiling a new layer of complexity in solar magnetic structure. Lead author Dr. David Kuridze calls them “the fingerprints of fine-scale magnetic field variations”.

Ultra-Fine Striations on the Solar Photosphere

According to the study, using DKIST's Visible Broadband Imager (VBI) in the G-band (430 nm), researchers captured fine stripes at ~0.03″ (~20 km) resolution. The images show alternating bright and dark bands on solar granule walls, each 20–50 km across. These patterns come from thin, curtain-like sheets of magnetic field rippling across the granule walls.

As Kuridze explains, stronger fields yield bright lanes and weaker fields dark lanes. Models show that ~100 gauss of field variation can create slight density dips (Wilson depressions) a few kilometers deep in the photosphere. At this fine scale, Kuridze notes, the striations are literally “the fingerprints of fine-scale magnetic field variations”.

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Implications for Solar Magnetism and Space Weather

Mapping this fine-scale magnetic architecture is crucial for understanding solar storms. Tiny surface fields can seed flares, eruptions and coronal mass ejections – events that drive space weather – so resolving them improves space weather forecasting. NSO co-author Dr. Han Uitenbroek points out that similar magnetically induced stripes have been seen in distant molecular clouds, highlighting the universal significance of this phenomenon.

With its 4-meter aperture – the world's largest solar telescope – DKIST was built to probe solar magnetism. Observers hail this discovery as “one of many firsts” for Inouye, underscoring DKIST's unique power to reveal the small-scale magnetic physics that drive space weather. DKIST was designed to resolve these fine magnetic features.

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