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uchicago.edu
The solar wind, explained
First proposed in the 1950s by UChicago physicist Eugene Parker, the solar wind is a flow of particles that comes off the sun at about one million miles an hour.
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Mar 10, 2021
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The solar wind, a stream of charged particles flows at 447 km/s (1 million mph), and while the magnetic field protects us,some particles still cause auroras and geomagnetic storms. | Science Of The Universe
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The solar wind – a constant stream of particles and energy flowing from the Sun – was first theorized 65 years ago. But that doesn’t mean scientists have uncovered all its secrets. In fact, a fresh look at data from 12 NASA spacecraft is giving scientists a new perspective. Scientists have long known there’s a lot of variability in the solar wind. Some days huge bursts of particles are released by solar flares, and other days there can be little activity. But how does the solar wind behave on av
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The Sun is constantly streaming charged particles toward Earth in what’s known as the solar wind. 🌞 Thankfully, Earth’s magnetic field acts like a giant umbrella, shielding our planet. But when the Sun and Earth’s magnetic fields connect and disconnect, they can explosively transfer energy, powering beautiful auroras and, at times, disrupting GPS, communications systems, and even posing risks to astronauts. Now, you’re invited to help NASA scientists study this dynamic region. With the new Spac
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The Sun (150.000.000 Km away) constantly releases a stream of charged particles called the solar wind. During solar flares or coronal mass ejections (CMEs), this stream intensifies, flooding space with high-energy particles. When those particles reach Earth, most are deflected by the magnetosphere, our planet’s magnetic shield. But near the magnetic poles, the field lines curve inward, guiding some particles into the upper atmosphere. There, they collide with atoms of oxygen and nitrogen, exciti
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