‘Space Waves’ Offer New Clues to Space Weather, Embry-Riddle Researchers Report
Research Associate Dr. Shiva Kavosi of Embry-Riddle (Photo: Shiva Kavosi)
More accurate space weather predictions and safer satellite navigation through radiation belts could someday result from new insights into “space waves,” researchers at Embry-Riddle Aeronautical University reported.
The group’s latest research, published on May 4, 2023, by the journal Nature Communications, shows that seasonal and daily variations in the Earth’s magnetic tilt, toward or away from the sun, can trigger changes in large-wavelength space waves.
These breaking waves, known as Kelvin-Helmholtz waves, occur at the boundary between the solar wind and the Earth’s magnetic shield. The waves happen much more frequently around the spring and fall seasons, researchers reported, while wave activity is poor around summer and winter.
As plasma or solar wind streams from the sun at speeds up to 1 million miles per hour, it pushes energy, mass and momentum toward the planet’s magnetic shield. It also whips up space waves.
Fast-moving solar wind can’t pass directly through the Earth’s magnetic shield, so it thunders along the magnetosphere, propelling Kelvin-Helmholtz waves with massive peaks up to 15,000 kilometers (km) high and 40,000 km long.
Astronaut Safety and Satellite Communication
“Through these waves, solar wind plasma particles can propagate into the magnetosphere, leading to variations in radiation belt fluxes of energetic particles — regions of dangerous radiation — that may affect astronaut safety and satellite communications,” said Dr. Shiva Kavosi, a research associate at Embry-Riddle and first author of the Nature Communications paper. “On the ground, these events can impact power grids and Global Positioning Systems.”
Dr. Katariina Nykyri, professor of physics and associate director for the Center of Space and Atmospheric Research at Embry-Riddle (Photo: Katariina Nykyri)
Describing the properties of space waves and the mechanisms that cause them to intensify is key to understanding and forecasting space weather, Kavosi noted: “Space weather events represent an increasing threat, yet in many cases, we don’t understand exactly what controls it. Any progress we can make in understanding the mechanisms behind space weather disturbances will improve our ability to provide forecasts and warnings.”
In trying to understand the causes of seasonal and diurnal variations of geomagnetic activity, researchers in the field have set forth several different hypotheses. For example, the Russell-McPherron (R-M) effect, first described in 1973, explains why auroras are more frequent and brighter in the spring and fall, based on the interplay of the Earth’s dipole tilt and a small magnetic field near the sun’s equator.
“We don’t have all the answers yet,” said Dr. Katariina Nykyri, professor of physics and associate director for the Center of Space and Atmospheric Research at Embry-Riddle, “but our paper shows that the R-M effect is not the only explanation for the seasonal variation of geomagnetic activities. Equinox-driven events, based on the Earth’s dipole tilt, and R-M effects could operate simultaneously.”
In the future, Nykyri added, constellations of spacecraft in the solar wind and magnetosphere could more fully explain the complicated, multi-scale physics of space weather phenomena. “Such a system would allow advanced warnings of space weather to inform the operators of rocket launches and electrical power grids,” she said.
The Nature Communication” paper concludes that “KH waves activity exhibit seasonal and diurnal variations, indicating the critical role of dipole tilt in modulating KHI across the magnetopause as a function of time.”
The research article, “Seasonal and Diurnal Variations of Kelvin-Helmholtz Instability at Terrestrial Magnetopause,” was authored by Embry-Riddle researchers Nykyri and Kavosi; C.J. Farrugia and Jimmy Raedar of the University of New Hampshire, Institute for the Study of Earth, Oceans and Space; and J.R. Johnson of Andrews University. The DOI is 10.1038/s41467-023-37485-x.
The work was supported by NASA grants (numbers 80NSSC18K0661, SA405826326 80NSSC18K1381, 80NSSC22K0304 and 80NSSC22K0515) as well as support from the Magnetospheric Multiscale mission (MMS) at the University of New Hampshire.