Skip to main content

Sun eruptions hit Earth like a 'sneeze', say scientists – University of Reading

Show access keys

Sun eruptions hit Earth like a 'sneeze', say scientists

Release Date 23 June 2017

CMEs are huge eruptions of solar plasma and magnetic fields from the sun's atmosphere

Long-term power cuts, destruction of electronic devices and increased cancer risk for aeroplane passengers are all potential effects of the Earth being hit by a powerful solar eruption.

Yet, new research has found space scientists have their work cut out to predict when these coronal mass ejections (CMEs) are on a collision course with Earth.

A study of CMEs by scientists at the University of Reading has found they have cloud-like structures. This means they are more influenced by solar wind, through which they pass to reach Earth, making their movements much harder to predict than if they were single bubble-like entities as was previously thought.

CMEs are huge blasts of solar plasma and magnetic fields from the sun’s atmosphere that can reach Earth in one to three days. A direct hit could have catastrophic consequences, as CMEs are capable of damaging satellites, destroying electronic devices and potentially exposing people at high altitude, such as astronauts and aviation crew and passengers, to cancer-causing radiation. They occur frequently, but predicting which ones will impact Earth and how severely is difficult.

Clouds not bubbles

Professor Mathew Owens said: “Up until now, it has been assumed CMEs move like bubbles through space, and respond to forces as single objects. We have found they are more like an expanding dust cloud or sneeze, made up of individual plasma parcels all doing their own thing.

“This means that trying to predict the shape and movement of CMEs as they pass through the solar wind becomes extremely difficult. Therefore if we want to protect ourselves from solar eruptions, we need to understand more about the solar wind.”

The new study, published in Nature Scientific Reports on Friday 23 June, looks in detail for the first time at how CMEs behave as they make their way through space, and how they interact with external forces like solar wind.

The Reading scientists took a cross section of a CME to examine its structure more closely. They found that a CME quickly reaches the point at which the speed of its expansion exceeds the speed at which information can travel within the CME. At this point, it ceases to be a coherent structure, so any distortion to one part of the cloud caused by external forces does not affect it as a whole.

Space weather threat

Scientists are constantly monitoring the sun to track solar wind and extreme space weather. The Reading team recommends that information about solar wind should be incorporated into CME observations to ensure we are fully aware of the threat they pose to Earth.

A previous study by University of Reading scientists found a shift in solar activity, expected to occur by the middle of the century, could make us more vulnerable to CMEs, as well as concentrating the Northern Lights around the poles – out of view of Great Britain.

In 2011, the threat of space weather was added to the Government National Risk Register of Civil Emergencies.


Full reference:

M.J. Owens, M. Lockwood and L.A. Barnard (2017). ‘Coronal mass ejections are not coherent magnetohydrodynamic structures’. Nature Scientific Reports. Doi: 10.1038/s41598-017-04546-3


Image credit: Nasa (2015)

We use Javascript to improve your experience on, but it looks like yours is turned off. Everything will still work, but it is even more beautiful with Javascript in action. Find out more about why and how to turn it back on here.
We also use cookies to improve your time on the site, for more information please see our cookie policy.