Billions of tons of plasma from the Sun are set to hit Earth today

A massive explosion on the surface of the Sun this week released billions of tons of plasma that are set to hit Earth today.

The eruption, known as a coronal mass ejection (CME), blasted off from the sun’s southwest region, sending plasma toward our planet with the help of the intense solar wind.

Forecast reports that there is a 50 percent chance that the particles will disrupt satellites in Earth’s orbit and a 10 percent risk of power outages.

The stream contains intense radiation that can interrupt technologies on Earth.

The solar wind is also expected to shake our planet’s magnetosphere, causing a G1 geomagnetic storm that could disrupt satellites orbiting in the area of ​​space.

A massive explosion ripping from the surface of the Sun was captured on April 24

The CME can eject billions of tons of corona matter from the sun’s surface. Matter consists of plasma and magnetic fields.

Such volcanic eruptions have the potential to spark space weather that can interfere with satellites and power grids on Earth and can be harmful to unprotected astronauts.

It was taken by the European Space Agency’s Solar and Heliospheric Observatory, which analyzes our Sun.

And just by fate, ejected coronal mass particles collide with Earth, as the stream was released from a coronal hole facing our planet.

Data from the National Oceanic and Atmospheric Administration (NOAA) shows that Earth’s magnetic field will malfunction around 6 p.m. ET tonight and could continue into Friday.

Earth’s magnetic field was ‘unstable’ as of Thursday and will continue for the next 24 hours as high-speed solar winds pour out of the coronal hole, EarthSky reports.

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Three coronal holes on the surface of the Sun face our planet and seven sunspots have been identified.

Sunspots are dark areas of the sun where it is cooler than other parts of the surface. Solar flares originate near these dark regions of the star.

Solar flares and coronal mass ejections come from these regions.

When it explodes toward Earth, it can trigger geomagnetic storms that produce beautiful aurorae and pose a threat to power grids and satellites.

SpaceWeather experts predict that over the next 24 hours, there is a 50 percent chance of C flares, a 10 percent chance of M flares and a 1 percent chance of X flares.

SpaceWeather experts predict that over the next 24 hours, there is a 50 percent chance of C flares, a 10 percent chance of M flares and a 1 percent chance of X flares.

This eruption, known as a coronal mass ejection (CME), pierced the sun's southwestern quadrant near a coronal hole, a cooler region on the surface.

This eruption, known as a coronal mass ejection (CME), pierced the sun’s southwestern quadrant near a coronal hole, a cooler region on the surface.

Thursday's sun also launched a cannibal CME on the northeast side of the solar disk facing away from Earth.

Thursday’s sun also launched a cannibal CME on the northeast side of the solar disk facing away from Earth.

Read more: Massive ‘solar hurricane’ swirls 74,500 miles high on sun’s surface

The tornado, made up of plasma and heat, reached more than 74,500 miles in height and traveled at 310,000 miles per hour.

Thursday’s sun also launched a cannibal CME on the northeast side of the solar disk facing away from Earth.

This type of cannibal will not affect our planet. He is turning away from us. SpaceWeather.com reports.

The sun is an amazing cosmic ball of gas that continues to surprise astronomers with its bewildering behavior.

One such incident was observed in February when a piece of the sun’s north pole was ripped off.

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Video shows a giant filament of plasma, or electrified gas, shooting out from the sun, separating and then spinning in a “massive polar vortex”.

While astronomers baffle, they speculate that the fame has something to do with a reversal of the sun’s magnetic field that happens once per solar cycle.

NASA describes solar filaments as clouds of charged particles that float above the sun, bound to them by magnetic forces.

These appear as elongated, uneven filaments projecting from the surface of the Sun.

“Once every solar cycle, it forms at about 55 degrees latitude and begins to travel toward the solar poles,” heliophysicist Scott McIntosh, deputy director of the National Center for Atmospheric Research in Boulder, Colorado, told Space.com.

He is very curious. There is a big “why” question. Why does it only move toward the pole once and then disappear and then return, magically, three or four years later in the exact same area?

While astronomers have previously observed filaments breaking away from the sun, this is the first time one has circled the region in a whirlwind.

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