The most powerful solar telescope on Earth reveals forces that drive solar storms

The Inouye Solar Telescope’s new tool, VTF, delivers sharp images of the Sun, helping scientists study eruptions and magnetic forces.

A powerful new solar telescope tool reveals the Sun’s surface and storms in sharper detail than ever before.

A powerful new solar telescope tool reveals the Sun’s surface and storms in sharper detail than ever before. (CREDIT: Youtube / CC BY-SA 4.0)

The Sun, an ever-burning ball of gas at the center of our solar system, has always fascinated people. But now, scientists are seeing it like never before. Thanks to the most powerful solar telescope on Earth, new doors are opening to unlock the Sun’s hidden behavior. This isn’t just about watching solar flares or counting sunspots. It’s about digging into the very forces that drive solar storms, which can knock out satellites and power grids on Earth.

The telescope making this leap is perched high above sea level, on a Hawaiian volcano named Haleakalā. From this prime location, researchers are gaining the clearest ground-based view of the Sun ever recorded.

A New Eye on the Sun

The Inouye Solar Telescope boasts a massive four-meter-wide primary mirror—the largest of its kind. This makes it unmatched in capturing the fine detail of the Sun’s surface and atmosphere. The dry, steady air above Haleakalā offers ideal conditions, letting this scientific giant operate with rare clarity. Since it started work in 2022, the telescope has delivered stunning close-ups of solar activity, revealing features only a few kilometers wide.

An image of a sun spot from the Daniel K. Inouye Solar Telescope. (CREDIT: U.S. National Science Foundation)

But its full power is just now being realized. The telescope is being equipped with specialized tools that break apart sunlight to examine its properties. Each instrument adds a layer of understanding. Four out of five planned instruments are now up and running. The newest and most powerful, the Visible Tunable Filter, or VTF, just took its first official image of the Sun.

This achievement marks what scientists call a “technical first light.” It means the instrument has captured its first scientific data, proving that it works as planned.

What Makes VTF So Special?

The VTF isn’t just another telescope part. It’s a groundbreaking tool with unmatched precision. Its mission is to capture the Sun’s light in extreme detail—splitting it into tiny slices of wavelength and even analyzing the way the light waves twist and turn. This helps scientists build detailed maps of the Sun’s surface and lower atmosphere.



To do this, VTF uses a pair of highly advanced devices called Fabry-Pérot interferometers. These filter the light down to wavelengths so precise, they measure just a few picometers—one trillionth of a meter. Each filtered slice of sunlight reveals different layers and features of the solar surface.

The result? Two-dimensional images of the Sun for each wavelength and each polarization of light. These images provide deep insight into the Sun’s temperature, pressure, plasma speed, and magnetic field strength at different heights above the surface.

“VTF enables images of unprecedented quality and thus heralds a new era in ground-based solar observation,” said Sami K. Solanki, a director at the Max Planck Institute for Solar System Research.

A Giant Heart for a Giant Telescope

The VTF is a technological beast. Weighing 5.6 tons and stretching across two floors, it takes up about as much space as a small garage. Engineers and scientists from an institute in Freiburg, Germany, developed it over a span of 15 years. They began installing it on the Inouye Solar Telescope in early 2024.

Inouye Solar Telescope. (CREDIT: AURA)

Matthias Schubert, the VTF project scientist, called this moment a major turning point. “The commissioning of VTF represents a significant technological advance for the Inouye Solar Telescope. The instrument is, so to speak, the heart of the solar telescope, which is now finally beating at its final destination,” he said.

That “heartbeat” is now sending a steady stream of high-speed, high-resolution images to scientists around the world. These images come at a pace of hundreds per second and show features as small as 10 kilometers across.

Understanding the Sun’s Explosive Behavior

The Sun may look calm from Earth, but it often erupts with violent storms. These solar storms send charged particles and radiation into space. When these reach Earth, they can cause glowing auroras near the poles. But they can also damage satellites, disrupt radio signals, and even affect power grids.

To predict such events, scientists must understand where and how these eruptions begin. The key lies in the Sun’s photosphere—its visible surface—and the chromosphere, the layer just above it. These zones hold a mix of swirling hot plasma and tangled magnetic fields. It’s this interaction that sparks solar eruptions.

This isn’t just about watching solar flares or counting sunspots. It’s about digging into the very forces that drive solar storms, which can knock out satellites and power grids on Earth. (CREDIT: NSO/NSF/AURA)

The VTF can now zero in on this region with unmatched clarity. By measuring magnetic field strength, pressure, flow velocity, and temperature, it gives scientists the tools they need to map out dangerous solar behavior before it reaches Earth.

“The Inouye Solar Telescope was designed to study the underlying physics of the Sun as the driver of space weather. In pursuing this goal, the Inouye is an ideal platform for an unprecedented and pioneering instrument like the VTF,” said Christoph Keller, Director of the National Solar Observatory.

A Look at the First Light

The first image from the VTF shows a sunspot in stunning detail. It uses sunlight at a wavelength of 588.9 nanometers and covers a part of the Sun’s surface about 25,000 kilometers wide. That’s roughly twice the size of Earth.

The image reveals a dark central spot with a finely woven outer region called the penumbra. These sunspots appear where strong magnetic fields stop hot plasma from rising, causing the surface to cool and darken. With a spatial resolution of 10 kilometers per pixel, the image lets scientists see the texture and structure of these magnetic regions with new depth.

NSO and KIS engineers and scientists work on the Visible Tunable Filter (VTF) inside the Coudé Lab at the Inouye Solar Telescope, preparing the instrument for its first light. (CREDIT: AURA)

Sunspots come and go in cycles that last about 11 years. Understanding how and why they form is critical to predicting solar storms. The VTF’s first image offers a promising glimpse into how scientists may soon track these patterns with greater accuracy.

Looking Forward

Though the telescope itself has been operational for a few years, the full power of its instruments is just coming online. With the VTF now in place, scientists can begin a new chapter of solar science. They’ll gain more accurate readings of solar conditions and better forecasts of solar activity.

For anyone on Earth who relies on GPS, satellite data, or electrical power—essentially everyone—this is good news. The Sun’s moods may not be easy to control, but they may soon be easier to predict.

Research findings are available online on the Max Planck website.

Note: The article above provided above by The Brighter Side of News.


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Mac Oliveau
Mac OliveauScience & Technology Writer

Mac Oliveau
Science & Technology Writer | AI and Robotics Reporter

Mac Oliveau is a Los Angeles–based science and technology journalist for The Brighter Side of News, an online publication focused on uplifting, transformative stories from around the globe. Passionate about spotlighting groundbreaking discoveries and innovations, Mac covers a broad spectrum of topics—from medical breakthroughs and artificial intelligence to green tech and archeology. With a talent for making complex science clear and compelling, they connect readers to the advancements shaping a brighter, more hopeful future.