Scientists utilize supercomputer simulations to examine the heated roots of the Sun to clarify the mysteries of solar moss

In this image provided by NASA’s High Resolution Coronal Imager sounding rocket, a small-scale structure on the Sun known as "moss" can be seen. Solar physicists refer to this patchy structure as moss and it appears in the lower part of the solar atmosphere around sunspot groups where magnetic activity is strong. The cooler roots of moss are shown in a detailed image from NASA’s Interface Region Imaging Spectrograph (IRIS) mission on the right. The credit for the image goes to NASA/Bose et al 2024.
In this image provided by NASA’s High Resolution Coronal Imager sounding rocket, a small-scale structure on the Sun known as "moss" can be seen. Solar physicists refer to this patchy structure as moss and it appears in the lower part of the solar atmosphere around sunspot groups where magnetic activity is strong. The cooler roots of moss are shown in a detailed image from NASA’s Interface Region Imaging Spectrograph (IRIS) mission on the right. The credit for the image goes to NASA/Bose et al 2024.

Cutting-edge research and supercomputer simulations reveal the mechanisms behind the heating of the enigmatic "moss" on the Sun's surface, providing new insights into the awe-inspiring power of our star.

In a groundbreaking scientific discovery, NASA scientists have made significant strides in unraveling the perplexing enigma of the Sun's "moss." This moss-like structure, a small-scale, patchy plasma formation in the solar atmosphere that shares an uncanny resemblance to earthly plants, has puzzled researchers for decades. However, thanks to the recent breakthrough enabled by NASA's High-Resolution Coronal Imager (Hi-C) sounding rocket and the Interface Region Imaging Spectrograph (IRIS) mission, combined with complex 3D supercomputer simulations, the mystifying puzzle is beginning to come together.

Named after its moss-like appearance, the region emerged into scientific consciousness back in 1999 through NASA's TRACE mission. Nestled within the center of a sunspot group and concealed beneath gossamer-like coronal loops, the moss straddles two atmospheric layers known as the chromosphere and corona, with engineers and scientists working tirelessly to unravel its secrets.

In the quest to understand the mechanism responsible for heating the moss, researchers have long been confounded by the extreme temperature disparity within this fascinating solar feature. While the surface just below the moss blazes at around 10,000 degrees Fahrenheit, the moss itself reaches blistering temperatures of nearly 1 million degrees Fahrenheit, defying conventional wisdom. Finally, through a combination of advanced observations and intricate 3D simulations, a remarkable discovery has been made.

The key insight derived from this comprehensive approach is the role of electrical currents. Within the moss region, an intricate web of magnetic field lines intertwines, akin to invisible spaghetti, generating electrical currents that contribute to heating the plasma. While the underlying mechanism responsible for this local heating is still not fully understood, this breakthrough represents a significant leap towards unraveling the broader question of why the Sun's corona is exponentially hotter than its surface.

"The convergence of high-resolution observations and advanced numerical simulations has allowed us to shed light on this 25-year-old mystery," shared Souvik Bose, a research scientist at Lockheed Martin Solar and Astrophysics Laboratory and Bay Area Environmental Institute, NASA's Ames Research Center. "But it is essential to note that this milestone only forms a fraction of the puzzle; the path ahead still holds numerous unanswered questions."

This groundbreaking discovery opens new avenues for further research and marks an inspiring turning point. The scientific community now stands poised to delve deeper into the secrets of our Sun, armed with an invigorated determination to unravel the mechanisms that govern its immense heat and energy.

However, this is just the beginning of an exciting journey. The quest to fully comprehend the interplay between the corona and the moss will require more observations and continued technological advancements. NASA's High-Resolution Coronal Imager (Hi-C) is set to launch again this month, adding another layer of understanding as it captures a solar flare and potentially additional moss regions in conjunction with the IRIS mission.

MUSE (MUlti-slit Solar Explorer), a promising future mission, is also on the horizon, with scientists and engineers working tirelessly to develop new instruments that will unlock even deeper insights into the enigmatic phenomena occurring on our Sun's surface.

The meticulous observations and cutting-edge supercomputer simulations offer not only a glimpse into the secrets of the Sun but also serve as a testament to the remarkable potential of human ingenuity. As we venture further into the exploration of space, these breakthroughs remind us that through the intertwining of diverse perspectives, innovative technologies, and unwavering curiosity, we have the power to unlock the mysteries of the universe.

Let these recent discoveries be a beacon of inspiration, underscoring the importance of investment in scientific research and space exploration. Together, we can embark on a journey to uncover the awe-inspiring intricacies of our celestial neighbor and expand our knowledge of the universe that surrounds us.