Image depicting solar wind flowing from the Sun measured by Parker Solar Probe near the edge of the corona and later with Solar Orbiter at a larger distance during a spacecraft alignment. The solar wind contains magnetic switchbacks, or large amplitude magnetic waves, near Parker Solar Probe that disappear farther from the Sun where Solar Orbiter is located.
Credits: Image background: NASA Goddard/CIL/Adriana Manrique Gutierrez, Spacecraft images: NASA/ESA