The world’s most powerful solar telescope on the sun sees incredible coronary loops (image)

When you buy through our articles links, Future and its syndication partners can earn commissions.

The smallest magnetic loops ever visible in the coron of the sun – for the first time, are displayed by the National Science Foundation Daniel F. Inouye solar telescope – can be the lower floor of machines that feed on cruel rings that usually blast our star.

“It’s an important moment of solar science,” said Cole Tamburri from Colorado University Boulder, a a statement; “We finally see the sun It works in the scales. “

In principle, Solar missiles are produced when the magnetic field lines originated through the outer atmosphere of the sun, the crownGrow tense and click, release energy before logging in again. It was known for a while, but the details associated with magnetic connection and sunlight still need a little training. One big question was: How small can these coronary loops be, and what role these miniature loops could play solar plaster?

Daniel K. Inouye Sun Telescope (DKIS), owned by the National Science Foundation (NSF) National Sun Observatory, has now depicted hundreds of coronary loops, which on average is just 29.95 miles (48.2 km), and some may be as thin as 13 miles (21 kilometers). This is directly by DKIS resolution, which is more than 2.5 times sharper than the other best solar telescope.

“Before Inouye, we could only imagine what this scale looked like,” said Tamburri. “Now we can see it directly.”

The small loop forest was visible in the light of hydrogen-alpha, seen by the visible broadband image after the X-Class exacerbation-to the most powerful exacerbation category, which can be released by the sun-measured 2024 m. August 8

“This is the first time the Inouye solar telescope has ever noticed an exacerbation of Class X,” said Tamburri. “These rockets are some of the most energetic events our star, and we are lucky to catch it in perfect observation conditions.”

It is not clear how these small loops play in the magnetic process process, but now that scientists know they are there, they can start to apply them to their models as the sun works. It is possible that these small loops are the main construction unit of the magnetic architecture of the sun, creating rackets.

“In this case, we not only solve the loop packages, but we also solve separate loops for the first time,” said the tamburri. “It’s like going from the forest to see every tree suddenly.”

The image of coronal loops shows the power of Inouye solar telescope, while the Tamburri itself is supported by the Inouye Sun Telescope Ambassador, funded by the NSF and aimed at the experience of young researchers they can enter into a wider sun community as they continue their careers.

But the clouds of storm gather on the horizon. The budget proposed by the US government for the 2026 fiscal year will allow Inouye solar telescope to receive a huge shortage of funding – from $ 30 million. USD up to $ 13 million Is not enough to open the Inouye solar telescope.

If the telescope should close, it would not only be the spectacular views of his sun, which we will lose, but also the experience of the researchers it helps to train. The loss of telescope and its scientists can be detrimental to the next year coming to the sun. However, if this is the last Inouye telescope, it goes high.

Tamburri and his team describe their observations about the small rackets released on August 25 Letters of astrophysical magazines;