An analysis using unprecedented satellite observations reveals important information about how electrons get heated throughout the Universe.
What connects solar flares that induce space weather, geomagnetic storms that cause auroras, and magnetic disruptions that spoil confinement in magnetically confined fusion devices? All these events rapidly convert stored magnetic energy into kinetic energy of surrounding electrons and positively charged ions in the plasma state of matter. The energy conversion occurs via a fundamental process called magnetic reconnection [1]. But some aspects of reconnection remain poorly understood, despite decades of scrutiny through theoretical studies, ground-and satellite-based observations, lab experiments, and numerical simulations [2]. A key unresolved problem is determining how much of the released magnetic energy goes to the electrons and how much goes to the ions, and by what physical mechanisms this energization occurs.