Sun is a source of energy in our solar system. Its surface is a violent and wild place. It is extremely challenging to touch the surface; still, we can have superb detail. Imagery from the Inouye solar telescope in Hawaii has revealed an explosive surface of the sun. The extraordinary striking images exhibit an amazing level of structure present inside the swirling plasma surface. The latest discovery has brought the formerly misty perception of the sun’s patchy surface intensely into attention initially. The telescope has a 30km resolution, which is more than double that of the future best solar interpretations.
Thomas Rimmele, the director of the mission, said these are the first-ever high-resolution images of the sun. He added, before this, they thought seemed like a bright dot, a single structure, but now it is decomposing into many smaller formations. The images expose the sun’s surface to be spotted with granule-like structures similar to chunks of gold. Even more, soaring columns of plasma, overheated to around 10,800F blow up as bright points at the middle of every grain. It seems like the center is powerfully releasing heat from the sun’s interior surface to the external one. As the plasma’s temperature gets low, it inclines back below the surface through thin, dark channels present between surrounding granules.
All in all, particulars in the newly-published images reveal plasma, that shields the sun and appears to boil. The world’s largest telescope, the Daniel K. Inouye Solar Telescope (DKIST) has made the things possible. The telescope’s peerless sensitivity and resolution will enable it to investigate the magnetic field of the sun. After that, the very first time it will assess the activities that control space weather near the Earth. Even more, charged particles coming from the sun can obstruct the communication set-up, power networks, and mechanical satellites of the Earth. The latest solar telescope will probe into one of the most illogical cosmic secrets. In other words, it will seek why the exterior layer of the sun is hotter than its face-up. Knowing the physics behind solar flares and CME (coronal mass ejections) could considerably enhance the ability to estimate whether in the space.