This study uses advanced computer simulations to model reconnection at the boundary of Earth's magnetosphere. Within this model, we fly a 'virtual spacecraft' through reconnection events to measure the local energy conversion rate. We test how our measurements are affected by different solar wind conditions and by the specific path our virtual probe takes through the event.

By comparing these results, we can better understand and validate the techniques used to analyze data from real spacecraft. This work is crucial for refining our understanding of how this fundamental process operates under various solar conditions, ultimately improving our ability to forecast space weather and protect critical infrastructure.