December 26, 2024

A solar strand 30 times longer than Earth is expected to hit us

2 min read
A solar strand 30 times longer than Earth is expected to hit us
NASA says that the solar filament is thirty times larger than the Earth should hit us today

NASA says that the solar filament is thirty times larger than the Earth should hit us today

  • The length of the fuse is 384,400 km;

  • This phenomenon can destroy satellites and destabilize power networks;

  • Solar monitors first spotted the filaments on July 12.

Experts have warned of powerful solar storms that could hit Earth today. According to them, a giant rupture Sun filaments Similar to the “Valley of Fire” can cause major disturbances, destroy satellites and destabilize power networks in different parts of the planet. The thread is 384,400 kilometers long, which, for comparison, is 30 times the size of Earth, which has a diameter of 12,742 kilometers.

The exploding solar filament will hit Earth directly today and is expected to cause a G-1 geomagnetic storm, with some experts suggesting that the storm could be much stronger in G-3. Fortunately, G-1 is the weakest form of geomagnetic storm, warning of NASA On weak fluctuations in the power grid and minor outages in satellite operations.

A G-3 geomagnetic storm is classified as strong and, according to NASA, would cause power outages and could jam satellites orbiting low Earth.

According to the site space climate, Solar observers first spotted the filaments on July 12, when they looked similar to filaments against a backdrop of a rising sun. Three days later, NASA’s Solar Dynamics Observatory recorded an eruption when “dark magnetic filaments spurted out of the Sun’s atmosphere, cratering a ‘giant valley of fire’,” experts from spaceweather.com wrote.

The choke traced the channel where the wire was suspended by magnetic forces above the sun’s surface before the instability released the solar flare directly toward Earth.

Solar filaments are giant filaments of electrified gas or plasma that float around the Sun’s atmosphere, influenced by its strong magnetic field. These unstable filaments often appear above sunspots, which are magnetically disturbed regions on the surface of the Sun.

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