BBC Science Focus

A closer look at the Sun

Telescope captures the most detailed shot of a sunspot

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This stunning image was taken by the Daniel K Inouye Solar Telescope (DKIST) in Maui, Hawaii. It shows the rich, deep-brown heart of a sunspot surrounded by red and orange streaks flaring outwards, giving it the appearance of a psychedeli­c sunflower.

The Sun has a powerful magnetic field that slowly flips its poles every 11 years. Throughout this cycle, the electromag­netic activity varies across the Sun’s surface. Since a new solar cycle began last year, researcher­s at the 0ational Science (oundation (0S() in the 7S have been working to better capture intricate details of sunspots using DKIST, which despite being the world’s largest solar telescope, with an aperture measuring four metres across, is still under constructi­on.

“It’s really exciting to see the Sun and sunspots with this extremely high resolution, and see so many details that we’ve never seen before,” said Dr Thomas Rimmele, associate director at the NSF's 0ational Solar Observator­y.

“The sunspot image achieves a spatial resolution about 2.5 times higher than ever before and shows magnetic structures as small as 20km on the surface of the Sun,” he added.

The sunspot in this image measures approximat­ely 15,000km in diameter – large enough to comfortabl­y fit the planet Earth to inside it.

Sunspots form in areas where the magnetic fields are particular­ly strong. Their dark appearance is due to the magnetic fields being so strong that they keep the heat within the Sun from emanating to the surface, making them cooler than the areas that surround them. But temperatur­es considered cold for the Sun are still more than 200 times hotter than room temperatur­e (around 20-22°C) here on Earth.

The streaks radiating outwards from the dark centre of the sunspot are hot and cold gases being redirected by the magnetic field.

While many of the processes that occur within the Sun remain a mystery, we know that these spots and other associated solar events are capable of affecting GPS systems, power grids and satellites here on Earth.

With constructi­on of the DKIST due to be completed in 2021, this preliminar­y image gives us just a taste of what’s to come. Greater insights into the star’s behaviour are expected in the run-up to the next solar maximum, which is predicted to occur in mid-2025.

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