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Some of the most hotly debated regions of Earth鈥檚 magnetic field are its cusps, located high above the Arctic and Antarctic on the sunlit side of the planet. These regions are where Earth鈥檚 magnetic field links up with the听, in an explosive process called听. The newly linked field lines form 鈥渇lux tubes鈥� that arc inward toward the poles, and the energy released from this process flicks charged particles zipping down them toward the poles. Thus, the cusps act as a portal for energetic particles in the, allowing them to penetrate听.

For decades, scientists have flown satellites through the cusp regions to study this process in detail at Earth. One of the defining characteristics is that the influx of dense plasma, including hot helium ions streaming off the Sun, pushes in on the planet鈥檚 magnetic field, depressing it toward the planet. Spacecraft can detect these events by a fall in magnetic pressure accompanied by a rise in plasma pressure, as well as higher densities of helium.

Recently, scientists have been able to study this process at Saturn, but the results are a bit different than at Earth.听听used observations from NASA鈥檚听, which crashed into Saturn听. Going back to data from 2007 to 2013, the team analyzed eight passes that the spacecraft made through the ringed planet鈥檚 cusps, tracking the changes in magnetic pressure and plasma pressure.

They found some broad similarities to Earth鈥檚 cusps: Whenever the magnetic pressure decreased, the plasma pressure increased, indicating that the plasma was pressing inward against the magnetic field. In addition, the stronger and faster the solar wind was, the bigger the indentation it made on Saturn鈥檚 magnetic field was.

Unlike at Earth, the magnetic depression wasn鈥檛 placed exactly in the center of the cusp; instead, it appears closer in to Saturn, butting up against particles trapped within the planet鈥檚 magnetic field. In fact, the plasma encountered by Cassini in that region isn鈥檛 just from the solar wind: Compositional analysis indicates that solar wind plasma mixes with plasma already present in Saturn鈥檚 magnetic field, which originates from the听听贰苍肠别濒补诲耻蝉.

Furthermore, although Cassini detected ionized helium in most of its passes through the cusp, there was no correlation between the amount of it and the depth of the magnetic depressions, as you would expect if the helium were part of the inflowing solar wind. Instead, it seems these helium ions are already there, trapped in Saturn鈥檚 magnetic field. This means that there must be some other way for helium to penetrate Saturn鈥檚 magnetic field besides reconnection at the cusp鈥攁n open question for future study.听