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Space.Fan — Go Beyond
ApJL · 7 DAYS AGO
Sun & Space WeatherNEW OBSERVATION

Sun's Magnetic Field Forms Hidden Canopy-Like Structures

By Space.Fan Editorial Desk

New high-resolution images show that the Sun's magnetic field acts like a giant umbrella, spreading out at the edges of magnetic patches.

Total solar eclipse with a brilliant white corona suspended above the curved horizon of Earth viewed from space.
Image · Space.Fan

The Drop

Scientists have captured a detailed look at the magnetic field of our Sun. By using a powerful instrument called the Sunrise III mission, they studied small, quiet patches on the Sun's surface. These patches, known as magnetic network elements, are like tiny magnetic anchors in the sea of the Sun's bubbling outer layer. What they found is that these magnetic fields do not just shoot straight out like a pillar. Instead, they fan out near the top of the Sun's atmosphere, creating a shape that looks like a canopy or an umbrella. This structure helps protect and organize the magnetic environment above the surface. To see this, the team used the Chromospheric Infrared SpectroPolarimeter, which allowed them to measure the magnetic field from the bottom of the solar atmosphere all the way up into the higher, hotter regions. They saw that the magnetic field is strongest around the edges of these patches, forming a ring. By tracking how the light from the Sun changes, the researchers proved that the magnetic field lines tilt and spread out as they reach higher levels of the Sun. They also noticed small, messy pockets of magnetic energy where the polarity—the north and south direction of the magnetic field—gets tangled up. These small, confusing spots show that the Sun's surface is more complicated than scientists previously thought.
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Why It Matters

This discovery is important because it shows us how the Sun's magnetism really works in 3D. Before now, scientists often used simpler models that treated these magnetic pillars as straight lines. Finding this 'canopy' shape helps us understand how energy moves from the surface of the Sun into its hot outer atmosphere, which is known as the corona. If we want to predict solar storms that could affect our technology on Earth, we need to know exactly how these magnetic structures are built and how they release energy.
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The Catch

While these observations provide a much clearer picture, they only look at a tiny portion of the Sun at one specific time. The Sun is massive, and its magnetic field is always changing, so it is hard to know if this canopy shape is the same everywhere or if it changes depending on the sunspot cycle. The researchers also noted that some parts of the data are very complex, making it difficult to tell exactly what is happening in the smallest, most tangled pockets of magnetism.

Put That in Perspective

In the past, our technology could not see the fine details of the Sun's magnetic field, leaving us to rely on educated guesses. The Sunrise III mission provides the sharpest view yet, acting like a magnifying glass for the Sun's surface. Researchers plan to use this data to refine computer models of the Sun to see if they can recreate these magnetic umbrellas in a digital environment.

Source September 1, 2026
ApJL

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