BBC NEWS Americas Africa Europe Middle East South Asia Asia Pacific
BBCi NEWS   SPORT   WEATHER   WORLD SERVICE   A-Z INDEX     

BBC News World Edition
 You are in: Science/Nature  
News Front Page
Africa
Americas
Asia-Pacific
Europe
Middle East
South Asia
UK
Business
Entertainment
Science/Nature
Technology
Health
-------------
Talking Point
-------------
Country Profiles
In Depth
-------------
Programmes
-------------
BBC Sport
BBC Weather
SERVICES
-------------
EDITIONS
Monday, 2 September, 2002, 14:58 GMT 15:58 UK
Sun gives up secrets
Coronal mass ejections (SOHO/LASCO consortium)
The huge ejections contain twisted solar material

The Sun spits out huge bubbles of super-hot electrified gas.

The solar eruptions blast out into space at speeds thousands of times faster than Concorde.

Sometimes they can even disrupt the Earth's magnetic field, leading to power black-outs.

Northern Lights (PA)
Northern lights in Canada's Arctic North
They are also behind the most dramatic spectacle in the sky - the northern (and southern) lights.

The colourful light shows happen when solar eruptions strike the region of space shielded by our planet's magnetic field.

But despite their impact on Earth, it is not known exactly how the Sun spews out the giant bubbles of gas, known as coronal mass ejections (CMEs).

Now UK astrophysicists have found new clues. They think twisted magnetic fields deep within our star could be the driving force.

The evidence comes from data gathered by the SOHO and Yohkoh satellites.

Twisted structures

Twists within the Sun's magnetic field were studied by a team at the Mullard Space Science Laboratory (MSSL) in Surrey.

One theory is these twisted structures are caused by the Sun rotating faster at the equator than the poles, says Dr Lucie Green of MSSL.

But the new study, carried out with colleagues in France and Argentina, suggests a second option is more likely.


Prediction of space weather is still a long way off

Dr Lucie Green, MSSL
"The magnetic field doesn't get twisted enough by the differential rotation that happens on the surface," Dr Green told BBC News Online.

"The implication is that the magnetic field must get twisted deep within the Sun itself."

Scientists hope it will one day be possible to predict when the Sun is likely to emit CMEs as part of space weather forecasts.

"Prediction of space weather is still a long way off but our research is helping us understand why CMEs happen in the first place," says Dr Green.

Main image courtesy of SOHO/LASCO consortium. SOHO is a project of international co-operation between the European Space Agency and NASA.

See also:

25 Jan 01 | Science/Nature
03 Mar 00 | Science/Nature
19 Feb 00 | Science/Nature
Internet links:


The BBC is not responsible for the content of external internet sites

Links to more Science/Nature stories are at the foot of the page.


E-mail this story to a friend

Links to more Science/Nature stories

© BBC ^^ Back to top

News Front Page | Africa | Americas | Asia-Pacific | Europe | Middle East |
South Asia | UK | Business | Entertainment | Science/Nature |
Technology | Health | Talking Point | Country Profiles | In Depth |
Programmes