Powerful Solar Storms Can Change Precipitation for Parts of North America
For decades, scientists have searched for a clear link between the Sun’s explosive storms and the weather that occurs on Earth.
Key points
- Focus: For decades, scientists have searched for a clear link between the Sun’s explosive storms and the weather that occurs on Earth
- Detail: Science reporting: verify primary technical documentation
- Editorial reading: science reporting; whenever possible, verify the cited primary source.
For decades, scientists have searched for a clear link between the Sun’s explosive storms and the weather that occurs on Earth. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.
That matters because Earth science becomes stronger when local observations can be placed inside a broader physical pattern that spans time and geography. The planet operates as a coupled system in which atmospheric, oceanic, cryospheric and solid-Earth processes interact across timescales from days to millions of years. A measurement that captures one variable at one location and one moment has limited interpretive value until it is embedded in the longer series and wider spatial coverage that allow natural variability to be separated from forced change. A breakthrough study from the University of New Hampshire reveals that in the hours and days following a solar storm, parts of North America can see sharp changes in the weather. But some of Nature's patterns are far more difficult to discern, and only after gathering data for decades do they reveal themselves.
But new research based on decades of data shows that the Sun's powerful storms can affect precipitation in the same day they reach Earth. It has long been a mystery why small Total Solar Irradiation changes have significant effects on Earth's climate" Raeder write.
Solar cycle correlation studies abound but cannot conclusively point to a viable physical mechanism. The data is from hourly Disturbance storm time (Dst) index and ERA5 atmosphere data for North America.
ERA5 is hourly data on Earth's global climate and weather that goes back decades, from 1940 onwards. ERA5 provides hourly estimates for a large number of atmospheric, ocean-wave and land-surface quantities," their website states.
The broader interest lies in linking the observation to climatic, geophysical or environmental dynamics that extend well beyond the immediate event or location. Earth science is unusual in that its most important questions operate on timescales that no single research career can observe directly, making the archival record, whether in ice, sediment, rock or satellite data, as important as any new measurement. Results that can be embedded in that record, and that either confirm or challenge the patterns it reveals, carry disproportionate scientific weight.
We’ve long understood that the sun influences our atmosphere over its roughly 11-year cycle, it’s subtle, but it’s there,” Raeder said in a press release. In this case, when a solar flare strikes Earth, the electromagnetic energy can penetrate into Earth's atmosphere via the polar vortex.
Because this item comes through Universe Today as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.
The next step is to place the result inside longer time series and to compare it with independent instruments and independent sites. Earth system observations gain most of their interpretive power from network density and temporal depth, not from any single measurement however precise. Model simulations that assimilate the new data will help clarify whether the observation fits comfortably within known natural variability or represents a shift that existing models do not reproduce.
Original source: Universe Today