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You WON'T BELIEVE What NASA Just Admitted - This Changes EVERYTHING
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Recently, the Sun experienced an extraordinary solar storm, which resulted in the formation of a massive fire canyon. This massive outburst of charged plasma was animated in stunning detail by NASA's Solar Dynamics Observatory. In April of 2022, charged particles from the sun finally reached Earth, and on August 9 following a solar flare, they did so again. They smashed at 600 km/s into the Earth's magnetosphere, creating auroras. The northern lights were visible from the United States to Canada. Scientists, though, think that our good fortune was simply a fluke this time around. Instead of a spectacular celestial show, it could have been disastrous had a more intense solar storm hit Earth. Solar storms have previously demonstrated their devastating potential at least twice in the past. The possibility of another strong burst of plasma from our Sun is increasing now that its activity is nearing its peak once again. Concerns have been raised about the Sun's current activity and the potential consequences of the next major solar storm for life on Earth. Make sure to stay until the end to know all there is to know about the unusual activity happening on the Sun right now!
The solar wind is a continuous stream of protons and electrons from the corona, the sun's outermost atmosphere. In a plasma state, these charged particles travel across the solar system at rates ranging from roughly 250 miles (400 kilometers) per second to 500 miles (800 kilometers) per second. When solar wind reaches Earth, it sends a flurry of charged particles into the magnetosphere and along Earth's magnetic field lines, causing them to collide and travel to the poles. The interaction of these particles with the Earth's atmosphere can result in spectacular aurora displays over the polar regions. The existence of the solar wind was first proposed by pioneering astrophysicist Eugene Parker. According to the University of Chicago, Parker was working as an assistant professor in 1957 when he recognized the sun's superheated corona should, in theory, release charged particles at high speeds. This superheating is one of the most enigmatic characteristics of the sun's activity, and solar physicists are still puzzled as to why the sun's atmosphere is hotter than its surface.
The solar wind is a continuous stream of protons and electrons from the corona, the sun's outermost atmosphere. In a plasma state, these charged particles travel across the solar system at rates ranging from roughly 250 miles (400 kilometers) per second to 500 miles (800 kilometers) per second. When solar wind reaches Earth, it sends a flurry of charged particles into the magnetosphere and along Earth's magnetic field lines, causing them to collide and travel to the poles. The interaction of these particles with the Earth's atmosphere can result in spectacular aurora displays over the polar regions. The existence of the solar wind was first proposed by pioneering astrophysicist Eugene Parker. According to the University of Chicago, Parker was working as an assistant professor in 1957 when he recognized the sun's superheated corona should, in theory, release charged particles at high speeds. This superheating is one of the most enigmatic characteristics of the sun's activity, and solar physicists are still puzzled as to why the sun's atmosphere is hotter than its surface.
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