High above the surface of Mars’s sunlit side, protons of the solar wind begin to smash into the upper reaches of Mars’s atmosphere. NASA’s Mars Atmosphere and Volatile Evolution Mission (MAVEN) spacecraft, which arrived at the Red Planet in 2014, has detected mysterious beams of oxygen ions flowing away from the planet, across the solar wind or even directly against it. Scientists have hotly debated how these counterstreaming beams form.
[A recent paper in the Journal of Geophysical Research — Space Physics by Kei Masunaga and coworkers] analyzed data from the MAVEN spacecraft. They found four examples of these fast beams of oxygen ions cutting through the solar wind upstream of Mars. By studying the velocity distributions of the ions, the team determined that they were carrying too much speed to have originated directly from Mars itself. Instead, oxygen atoms in the extended exosphere are ionized before they reach Mars, streak in with the solar wind, and are then repelled back outward at speed. (…)
The team’s analysis shows that the oxygen ions penetrate the bow shock, but as they sink toward the surface of the planet, the piled-up magnetic and electric fields cause them to turn 180° and fling them back out into the solar wind — possibly even escaping Mars. [More at links]