By estimating the effect of the solar wind on any one CME, the team said it suffices to then gauge the ejections initial velocity to forecast when it might arrive at Earth.
The team created the model by comparing historic data collected by satellites positioned both on and off the sun-Earth line. That allowed them to accurately measure both the initial velocity of CMEs at the sun, thanks to the satellites that viewed the events in profile, and the velocity of the ejections far from the sun in Earths vicinity.
The combined measurements gave the team the change in the CMEs velocity attributable to the influence of the solar wind.
The team, which included scientists from NASAs Goddard Space Flight Center, used the technique to predict within six hours when a June 6 ejection would arrive at Earth. Further work should refine the model, allowing even more precise forecasts.
Ernest Hildner, director of the National Oceanic and Atmospheric Administrations Space Environment Center, heralded the model.
"This result announced today gives us a new opportunity to determine the onset time of any particular storm," Hildner said.
The team presented the study results during a press conference held Monday at a meeting of the Solar Physics Division of the American Astronomical Society at Lake Tahoe, Nevada.
Future space missions, like NASAs Solar-Terrestrial Relations Observatory (STEREO) will use a pair of satellites to view Earth-directed CMEs in three dimensions, allowing scientists to precisely pinpoint their velocity.