Plasma, the ionised state of matter found in stars, is still not fully understood. Astrophysicists have long-since sought to develop models that can account for the turbulent motions inside plasma. Turbulences are typically detected through observation of broadened lines due to the Doppler Effect. In a new study, researchers have developed an iterative simulation model that accurately predicts changes to the line shape in the presence of strong plasma turbulence.
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