What is the sun really like? Telescope captures the most detailed images to date of its surface

<p class = "canvas-atom canvas-text Mb (1.0em) Mb (0) – sm Mt (0.8em) – sm" type = "text" content = "Due to the distance between the Earth and the Sun –149.6 million kilometers–, the star may seem to us only a sphere that emits light. But the high-resolution images and videos captured by a telescope in Hawaii remind us that there is an incessant activity on the solar surface. “Data-reactid =” 31 “> Due to the distance between the Earth and the Sun –149.6 million kilometers–, the star may seem to us only a sphere that emits light. But the high-resolution images and videos that a telescope captured in Hawaii remind us that there is an incessant activity on the solar surface.

<p class = "canvas-atom canvas-text Mb (1.0em) Mb (0) – sm Mt (0.8em) – sm" type = "text" content = "In hypnotists images from the Daniel K. Inouye Solar Telescope of the National Science Foundation is the “boiling” turbulent plasma that covers the entire Sun, “a star that burns 5 million tons of hydrogen fuel per second for billions of years.” data-reactid = “32”> In hypnotists images from the Daniel K. Inouye Solar Telescope of the National Science Foundation is the “turbulent‘ boiling ’plasma that covers the entire Sun”, a star that burns 5 million tons of hydrogen fuel per second for billions of years.

<p class = "canvas-atom canvas-text Mb (1.0em) Mb (0) – sm Mt (0.8em) – sm" type = "text" content = "Structures in the form of cells that appear in the captures are the size of Texas and are the record of movements that transport heat from inside the Sun to its surface. These then rise in the centers, cool and then sink below the surface, in a process known as convection. “Data-reactid =” 53 “> Structures in the form of cells that appear in the captures are the size of Texas and are the record of movements that transport heat from inside the Sun to its surface. These then rise in the centers, cool and then sink below the surface, in a process known as convection.

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<p class = "canvas-atom canvas-text Mb (1.0em) Mb (0) – sm Mt (0.8em) – sm" type = "text" content = "This 4-meter solar telescope allows you to measure and analyze the sun's magnetic field in detail, something that will help to understand this star and the impacts it causes on our planet the magnetic eruptions that can affect air transport, interrupt satellite communications and tear down networks. “data-reactid =” 54 “> This 4-meter solar telescope allows you to measure and analyze the Sun’s magnetic field in detail, something that will help you understand this star and the impacts it causes on our planet the magnetic eruptions which can affect air transport, interrupt satellite communications and tear down networks.

“We can share these images and videos, which are the most detailed of our Sun to date,” said France Córdova, director of NSF.

“The NSF Inouye Solar Telescope will be able to map the magnetic fields inside the Sun’s corona, where solar eruptions occur that can affect life on Earth. The telescope will improve our understanding of what drives space weather and, ultimately, will help predict solar storms better, ”he added.

The NSF explained in its statement that the telescope has a 4-meter mirror and is at the Haleakalā summit 3 kilometers away and has a specialized cooling system due to the amount of solar energy it generates.

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