The orbit of solar energy captures the first clear view of the southern pole of the sun – a hot chaos

For more than 60 years, many spacecraft and telescopes have traveled across space to stare at the sun, taking painful pictures of the giant ball of hot gas in the heart of our solar system. However, our point of view of the star is limited by the tropical plane, which allows us to monitor the equator in the sun while its polar areas remain in a frustrating blind place. Solar Orbiter is now the first to photograph the columns from outside the eclipse, providing a rare look at its chaotic magnetic field.

On Wednesday, European Space Agency (ESA) Absolute The first clear pictures of the southern pole of the sun, and revealed that both the northern and southern magnetic poles are currently on the same side. The new photos will help scientists understand the 11 -year magnetic cycle Magnetic storms on the ground.

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The orbit of solar energy used momentum from the Venus Fly on February 18 to push itself from the fracture level that contains the Earth’s orbit around the sun. About a month later, the spacecraft managed to watch the star from 17 degrees below the solar equator, enough to get a good view of the southern pole of the sun for the first time.

“We did not know exactly what to expect from these first notes – the sun’s columns are literally from the hidden Terra,” said Sami Solanki, who leads the solar roles crew in Germany.

The science team used three tools on the solar plane to take pictures of the sun between 16 and 17 March. Each sun instrument is noticed in a different way; The polarization and the seductive images (phi) take the sun in visible light, depicts extremist UV photographs (EUI) in UV rays, and discovers the spectral tool of the coronary environment (spices) the light emitted from the charged gas above the surface of the sun.

By combining the powers of viewing for all three tools, scientists have noticed the Southern Pole of the sun in the turmoil. Usually, each polar region has its own magnetic field properties. With the sun reaching a period of maximum solar energy during a 11 -year -old cycle, its magnetic polarity turns, with the reflection of the northern and southern magnetic poles. During the sun’s orbit notes, there is a polarity from the north and the south in the Antarctic.

This is an important time in understanding sun activity. After the magnetic field has passed, one polarity slowly accumulates in the columns of the sun and takes responsibility. When the sun reaches the minimum solar energy within about five to six years, each of the northern and southern columns will have its own magnetic polarity. “How this accumulation remains exactly incomprehensible, so the oriental or solar oriental orientation has reached high time lines in time only to follow the entire process from its unique and useful perspective,” Solanki said.

Scientists have used the task to measure how the sunlight groups move across the surface of the sun. Using the Doppler effect, which describes the changes in the frequency of light or sound during its move or the source, the team created a speed map showing how the speed of the material varies between the columns of the sun and the tropical region. With the help of the orbit of solar energy, scientists will gain a better understanding of the reason for the solar wind travel faster in the poles more than the equator in the sun.

Solar orbits have just started. Modern notes are the first collection of pictures taken from the newly tilted orbit of the spacecraft, but the spacecraft is preparing for another Venus Flyby on December 24, 2026, which will increase its orbit to 23 degrees below the equator to get a better vision of the sun.

“This is only the first step from” the stairs to the sky “from solar energy: in the coming years, the spacecraft will climb more than the fracture level for better views of the polar areas of the sun.” “This data will turn our understanding of the magnetic field of the sun, solar winds and solar activity.”