Scientists have mapped and recreated solar bursts in 3D using three NASA satellites, an advance that may help predict how such events may affect weather around Earth, endanger spacecraft and astronauts.
The new models can help see how shocks associated with coronal mass ejections (CMEs) propagate from the Sun by combining data from three satellites to produce a much more robust mapping of a CME than any one could do alone.
Much the way ships form bow waves as they move through water, CMEs set off interplanetary shocks when they erupt from the Sun at extreme speeds, propelling a wave of high-energy particles.
These particles can spark space weather events around Earth, endangering spacecraft and astronauts.
Understanding a shock’s structure — particularly how it develops and accelerates — is key to predicting how it might disrupt near-Earth space.
However, without a vast array of sensors scattered through space, these things are impossible to measure directly.
Instead, scientists rely upon models that use satellite observations of the CME to simulate the ensuing shock’s behaviour.
Researchers from George Mason University and Johns Hopkins University in the U.S. pulled observations of two different eruptions from three spacecraft: ESA/NASA’s Solar and Heliospheric Observatory (SOHO) and NASA’s twin Solar Terrestrial Relations Observatory (STEREO) satellites.
One CME erupted in March 2011 and the second, in February 2014.
The scientists fit the CME data to their models — one called the “croissant” model for the shape of nascent shocks, and the other the “ellipsoid” model for the shape of expanding shocks — to uncover the 3D structure and trajectory of each CME and shock.
Each spacecraft’s observations alone were not sufficient to model the shocks. However, with three sets of eyes on the eruption, each of them spaced nearly evenly around the Sun, the scientists could use their models to recreate a 3D view.
The study, published in the Journal of Space Weather and Space Climate , confirmed long-held theoretical predictions of a strong shock near the CME nose and a weaker shock at the sides.
In time, shocks travel away from the Sun, and thanks to the 3D information, the scientists could reconstruct their journey through space.
The modelling helps scientists deduce important pieces of information for space weather forecasting — in this case, for the first time, the density of the plasma around the shock, in addition to the speed and strength of the energized particles.
All of these factors are key to assessing the danger CMEs present to astronauts and spacecraft.
