'Internet blackout' that could last for months is avoided thanks to NASA mission

The pioneering Parker Solar Probe (PSP) mission from NASA achieved a significant milestone by successfully crossing the solar wind. This achievement aims to protect internet connectivity on Earth.

Little by little, we became even more independent of the use of the internet. Can you imagine what our life would be like in this apocalypse?

Scientists have warned of the impact of the solar storm on communication, known as the "internet apocalypse", which is expected for years to come.

By exploiting the solar wind, PSP aims to provide valuable information to understand and predict better these solar storms and mitigate their potentially damaging effects on Earth's infrastructure. Internet.

Professor Stuart Bale, lead author of the study and affiliated with the University of California, United States, highlighted the importance of understanding the solar wind.

Exploring this little-known region is essential to advancing our understanding of solar physics and the solar phenomena that affect our planet.

Solar wind plays a crucial role in the formation and evolution of space weather, and can trigger solar storms and affect communications, technology and power grids on Earth.

PSP mission saved us from a possible period without internet

The publication of the results of the Parker Solar Probe mission in the renowned journal Nature represents a breakthrough significant in the ability to predict solar storms and their impacts on communications, satellites and networks electrical.

According to the study, the scientists discovered that the coronal holes work like real showers, with jets of energy emerging from bright spots where magnetic field lines bend in and out of the surface solar.

The team of researchers described the experience as "watching jets of energy come out of a shower and hit your face." These observations were key to understanding “supergranulation flows” within coronal holes, regions where magnetic fields originate.

These regions appear to play a crucial role in generating the high-speed solar wind. Although coronal holes are normally found at the sun's poles during periods of calm, they have no direct impact on Earth.

The findings represent a fundamental piece in the puzzle of solar behavior and provide valuable information to improve our ability to predict and understand solar storms.

With a better understanding of these phenomena, we can better protect our critical infrastructure and ensure an effective response to intense solar events.

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