phenomenon

solar storm

A cloud of magnetized gas ejected from the Sun that can disturb the interplanetary medium.
17 related articles

Description

A solar storm, also known as a coronal mass ejection (CME), is a massive burst of magnetized plasma and radiation released from the Sun's corona into space. These clouds of charged particles can travel at speeds of hundreds to thousands of kilometers per second, and when they reach Earth, they interact with the planet's magnetic field, potentially causing geomagnetic storms. Such storms can disrupt satellite operations, power grids, and communication systems, and they are also responsible for the spectacular auroras seen at high latitudes.

History

The connection between solar activity and geomagnetic disturbances was first established in the mid-19th century, notably by Richard Carrington who observed a solar flare in 1859 that was followed by a major geomagnetic storm. The term 'coronal mass ejection' was coined in the 1970s after observations from the Skylab space station.

How it works

Solar storms originate from regions of intense magnetic activity on the Sun's surface, such as sunspots. When magnetic field lines become twisted and stressed, they can suddenly reconnect and release enormous amounts of stored energy, propelling a cloud of plasma outward. As this cloud travels through space, it carries with it the Sun's magnetic field. Upon arrival at Earth, the interaction between the solar magnetic field and Earth's magnetosphere can compress the magnetosphere on the day side and stretch it on the night side, leading to the injection of energetic particles into the upper atmosphere and the generation of strong electrical currents in the ionosphere.

In practice

Monitoring solar storms is crucial for protecting satellites, power grids, and aviation communications. Space weather forecasting agencies track CMEs to issue warnings, allowing operators to take preventive measures like shutting down sensitive electronics or adjusting satellite orbits.

Fun fact

The 1859 Carrington Event produced auroras so bright that people could read newspapers at night as far south as the Caribbean, and telegraph systems failed or sparked even when disconnected from their power sources.

Related articles · 17

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