Space Weather: The Sun’s Invisible Storms
- Mark Armstrong
- Feb 1
- 2 min read
While we usually think of "weather" as something happening in our atmosphere—like rain, wind, or snow—some of the most impactful weather on Earth actually originates 93 million miles away. Known as Space Weather, these solar phenomena are driven by the Sun’s magnetic activity. As we move through the active peak of the current Solar Cycle, understanding these cosmic forces has become increasingly critical for our high-tech society.

Space weather isn't about clouds or moisture; it’s about radiation and plasma. The Sun constantly emits a "solar wind," but during periods of high activity, it can produce much more violent eruptions:
Solar Flares: These are sudden, massive explosions of light and X-rays. Traveling at the speed of light, they reach Earth in just eight minutes. Flares primarily cause "Radio Blackouts," disrupting high-frequency communications used by pilots, mariners, and emergency responders. Today, active region AR4366 produced an X8.1 flare, causing significant radio interference across the Pacific.
Coronal Mass Ejections (CMEs): If a flare is the "muzzle flash" of a cannon, a CME is the "cannonball." These are giant clouds of billions of tons of solar plasma and magnetic fields. They travel slower than light, taking one to three days to reach Earth. When they arrive, they slam into our planet's magnetic shield, triggering a Geomagnetic Storm.
The Sun operates on an 11-year cycle. After a quiet "Solar Minimum" in 2019, activity has been ramping up toward a peak expected right now, in early 2026. This means we are seeing more sunspots—the dark, magnetically tangled regions on the Sun—which serve as the launchpads for these storms.
In fact, just this past month, in January 2026, Earth experienced a Severe (S4) Solar Radiation Storm, one of the most intense recorded since 2003. This event forced airlines to reroute flights away from polar regions and prompted satellite operators to place sensitive electronics on high alert to protect them from damage caused by high-energy particles.
You might not feel a solar storm when you walk outside, but your technology certainly does.
The Grid: Geomagnetic storms can induce "ghost currents" in long-distance power lines. Without careful management by grid operators, these surges can overheat and destroy massive transformers, leading to widespread blackouts.
GPS and Navigation: Space weather can "puff up" the Earth’s upper atmosphere, slowing or deflecting signals from GPS satellites. This can lead to errors for everything from your smartphone maps to autonomous tractors in precision farming.
The Aurora: On the bright side, these storms create the Aurora Borealis (Northern Lights). During powerful storms, these dancing lights have been visible much further south than usual, reaching into the mid-latitudes of the U.S. and Europe.
As our world becomes more dependent on satellites and digital connectivity, space weather forecasting is no longer just for scientists—it’s for everyone.






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