Nearly two years ago and about four months after launch on June 15, 2020made his first visit ” about “ from our . Probe ( , ) then traveled 77 million kilometers from our star. About half the Earth-Sun distance. A great opportunity, especially for researchers, to test ten instruments on board the vehicle. But the goal has not yet been reached.
Since then, Solar Orbiter has benefited from several operationsrelying on our Earth and Venus to finally get within a third of our star this Saturday, March 26, 2022 . Or about 48 million kilometers of just its seething surface. Thus, the probe penetrated the solar corona. And all of his ten instruments worked great, collecting data and images of our sun like never seen him before.
Over the next few years, Solar Orbiter will make several passes near our star. Of course, sending valuable information to researchers, especially since the probe will also be more and more focused on. Regions that have rarely been observed.
Sun in extraordinary resolution
Pending the publication of these unpublished photos and that they will reveal some more of the secrets of our star, the researchers working on the Solar Orbiter mission are already sharing the imagebreathtaking. About 83 million . The resolution is ten times better than our 4K screens. Simply put, the best image of the corona and the entire disk of our Sun ever taken.
The picture was taken March 7th. UsingExtremeImage (EUI) when Solar Orbiter was about half the distance from the Earth to the Sun. An image, or rather an image. Because the spatial resolution of the EUI is such that at 75 million kilometers it takes 25 images to cover the entire surface of our Sun. At a rate of about ten minutes for each shot, it took the probe at least four hours to perpetuate our star in this way.
Since it is in the extreme ultraviolet range that the EUI observes our Sun,out of 17 astronomers will be able to receive information from high our star. The environment in which goes up to about a million .
Another selection of amazing images
The tool called Spectral image of the coronal medium (SPICE) also returned exceptional images. The first of its kind in 50 years. And in fact, by far the best.
The device is designed to penetrate through the layers of the solar atmosphere, from the corona inward, to– by analyzing wavelengths extreme ultraviolet radiation from various . I’ gas at a temperature of about 10,000°C, here in purple at around 32,000 °C, blue, at a temperature of about 320,000 ° C, in green, and at a temperature not lower than 630,000 ° C, yellow. What to allow trace observed in the crown down to the lower layers . And, perhaps, to finally understand why the temperature increases in a completely illogical way as we move away in the solar atmosphere from the surface of our star.