Scientists have discovered the role of Alfvén waves in energizing the solar wind.
Alfvén waves carry energy from the Sun’s corona and are critical players.
High-amplitude Alfvén waves manifest as switchbacks observed during the probes' close encounters with the Sun.
These waves drive work on the plasma, item transferring energy that accelerates and heats the solar wind.
The breakthrough came in February 2022 when both probes serendipitously aligned to study the same stream of solar wind.
Parker Solar Probe detected switchback-rich slow plasma, while Solar Orbiter recorded a fast-moving, heated wind devoid of fluctuations.
Observations confirmed that Alfvén waves in the form of switchbacks provide enough energy to account for unexpected heating and acceleration of solar wind.
Understanding the mechanics of solar wind is important for predicting space weather, which can disrupt satellites, power grids, and communication systems on Earth.
This research could help in understanding how the winds and planetary systems influence the environments of other stars, making planets habitable.
The study underscores the importance of collaborative missions like Parker Solar Probe and Solar Orbiter.