This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: A new study led by researchers at the University of Oulu in Finland sheds light on a poorly understood part of space weather: where powerful waves form at the edge of Earth's magnetic shield and where the solar wind can find a way through. The study "IMF By-Controlled Dawn–Dusk and Hemispheric Asymmetries of Kelvin–Helmholtz Waves and Reconnection Geometry Under Negative Dipole Tilt" is published in Geophysical Research Letters.
Earth is surrounded by a magnetic field that forms a protective region known as the magnetosphere. It shields the planet from particles and energy streaming from the sun, a flow called the solar wind. But the shield is not sealed.
At its outer edge, the solar wind constantly interacts with Earth's magnetic environment. These interactions help drive space weather. On Earth, their effects can appear as auroras, but strong solar storms can also disturb satellites, positioning systems, radio communications and power grids.
The new study focuses on the wave motion that forms where the fast-moving solar wind brushes past the edge of the magnetosphere. The waves are known as Kelvin–Helmholtz waves. Similar wave patterns can sometimes be seen in clouds, and related phenomena occur in the sun's atmosphere, at the edges of other planets' magnetic fields and in interstellar space.
"This finding grew out of a long process of thinking through what I was seeing. In 2020, when I was visiting NASA as a postdoctoral researcher, I noticed unusual simulation images of the magnetosphere. I later realized that they showed Kelvin–Helmholtz waves at the edge of the magnetosphere and that the different behavior of the waves on different sides was part of the same phenomenon," says academy research fellow Lauri Holappa from the University of Oulu.
The waves do not form as neat mirror images. Instead, they appear asymmetrically on different sides of the magnetosphere. Studying these boundary waves is challenging because satellites pass through the most active regions only rarely.
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