Space Travel News  
SOLAR SCIENCE
Scientists See Solar Outburst In Exquisite Detail

A visible light image of the CME as it travelled from the Sun towards the Earth on 20 March 2010 made with the HI instrument on the STEREO observatory. The x-axis of the image corresponds to a distance of 48 million km from left to right. Credit: Anthony Williams / NASA / Richard Harrison
by Staff Writers
London, UK (SPX) Apr 20, 2011
The largest disturbances to the Earth's geomagnetic environment occur when it is buffeted by solar material hurled in our direction by explosive changes in the Sun's atmosphere. These Coronal Mass Ejections or CMEs contain approximately a billion tonnes of ionized gas or plasma and can have a dramatic and damaging impact on everything from satellites to power grids.

Now a team of scientists have used two spacecraft to study these events in unprecedented detail. Graduate student Anthony Williams of the University of Leicester will present their results at the Royal Astronomical Society's National Astronomy Meeting in Llandudno, Wales.

Mr Williams and his team used the Heliospheric Imagers (HI) on the Solar TErrestrial RElations Observatory (STEREO) spacecraft to examine the internal structure of an Earth-impacting CME - seen as sunlight scattered from high density blobs of plasma - as it travels outwards from the Sun.

They compared this with the internal structure measured in situ by the Advanced Composition Explorer (ACE) spacecraft as the CME engulfed the spacecraft and impacted the Earth. This meant that the scientists have for the first time been able to compare the evolution of the CME structure as it races towards the Earth and the internal structure observed as it arrives.

The CME studied was ejected from the Sun on 19 March 2010, when the STEREO A spacecraft was in a position to watch from the side as the CME hurtled outwards towards the Earth.

The structure of the CME was examined in HI images spanning a distance of approximately 48 million km at different distances between the Sun and the Earth. Analysing the images indicated that its speed was close to 350 km per second, which allowed its time of impact on the Earth to be predicted some 3 days after the initial ejection.

The results indicate that the CME structure evolves considerably on its outward journey, and that the internal structure can be difficult to predict from the images. And there is another key facet to this work - imaging CMEs with spacecraft like STEREO is an extremely effective means of forecasting their impact on Earth and the large scale disruption that can sometimes result.



Share This Article With Planet Earth
del.icio.usdel.icio.us DiggDigg RedditReddit
YahooMyWebYahooMyWeb GoogleGoogle FacebookFacebook



Related Links
Royal Astronomical Society
Solar Science News at SpaceDaily



Memory Foam Mattress Review
Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News


SOLAR SCIENCE
The Watched Pot And Fast CMEs
Greenbelt MD (SPX) Apr 18, 2011
Back in 2008, the solar cycle plunged into the deepest minimum in nearly a century. Sunspots all but vanished, solar flares subsided, and the sun was eerily quiet. "Ever since, we've been waiting for solar activity to pick up," says Richard Fisher, head of the Heliophysics Division at NASA Headquarters in Washington DC. "It's been three long years." Quiet spells on the sun are nothin ... read more







SOLAR SCIENCE
Ariane rocket launches two telecoms satellites

Ariane 5 Cleared For Launch With Yahsat Y1A And Intelsat New Dawn

SpaceX aims to put man on Mars in 10-20 years

PSLV Success Lifts ISRO Gloom

SOLAR SCIENCE
Dry ice find hints Mars was a wetter place: study

A Tale Of Two Deserts

Mars Rover's 'Gagarin' Moment Applauded Exploration

Mars Flight Possible After 2035

SOLAR SCIENCE
BRP To Contribute To Canadian Moon And Mars Exploration Programs

Naveen Jain Co-Founder And Chairman Of Moon Express

Project Morpheus To Begin Testing At NASA's Johnson Space Center

NASA Announces Winners Of 18th Annual Great Moonbuggy Race

SOLAR SCIENCE
Carbon monoxide detected around Pluto

The PI's Perspective: Pinch Me!

Later, Uranus: New Horizons Passes Another Planetary Milestone

Can WISE Find The Hypothetical Tyche In Distant Oort Cloud

SOLAR SCIENCE
The Shocking Environment Of Hot Jupiters

Radio signals could 'tag' distant planets

Titan-Like Exoplanets

A New Way To Find Planets

SOLAR SCIENCE
NASA awards $270 million in spaceship contracts

No Fleet Future For X-37B

Model Of Russian Piloted Spacecraft To Go On Show In August

100-Year Starship Study Strategic Planning Workshop Held

SOLAR SCIENCE
Asia's star ever brighter in space

What Future for Chang'e-2

China setting up new rocket production base

China's Tiangong-1 To Be Launched By Modified Long March II-F Rocket

SOLAR SCIENCE
Fast-Rotating Asteroid Winks For Astronomer's Camera

Cold Asteroids May Have A Soft Heart

WISE Mission Spots 'Horseshoe' Asteroid

WISE Mission Spots Horseshoe Asteroid


The content herein, unless otherwise known to be public domain, are Copyright 1995-2010 - SpaceDaily. AFP and UPI Wire Stories are copyright Agence France-Presse and United Press International. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by SpaceDaily on any Web page published or hosted by SpaceDaily. Privacy Statement