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STEREO L-1 Science Briefing
10.19.06
 
Presenter #1 - Mike Kaiser, STEREO Project Scientist, NASA Goddard Space Flight Center


Still from Mike Kaiser's video
Click image to view animation.


Still from Halloween storms LASCO C3 image animation of Solar flares and coronal mass ejections (CMEs)


Image #1 (left):The Solar and Heliopsheric Observatory (SOHO) watched CMEs streaming out into space during the notorious Halloween storms in October/November 2003. Click on the above image to play small movie (mpg) or view 640x480 version. Credit: NASA/ESA. Image #2 (right): Solar flares and coronal mass ejections (CMEs), associated giant clouds of plasma in space, are the largest explosions in the solar system. They are caused by the buildup and sudden release of magnetic stress in the solar atmosphere above the giant magnetic poles we see as sunspots. CMEs can cause magnetic storms affecting communication systems, power grids and astronauts in space. Click on image to view movie. Credit: NASA.

Artist's image of the STEREO spacecraft with instruments


Image #3 (left): Model of the STEREO observatory shows each of the instruments. Click image to enlarge. + Click for 8.7 MB tif Credit: NASA/APL.

Presenter #2 - Russ Howard, SECCHI Principal Investigator, Naval Research Laboratory (NRL)


Still from Russ Howard's video
Click image to view animation.


STEREO diagram 3
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Image #1 (above): SECCHI Instrument - The Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) will hve four instruments: an extreme ultraviolet imager, two white-light coronagraphs and a heliospheric imager.

Still from animation of the SECCHI instrument deployment.
Click image to view animation.

Image #2 (above): SECCHI deploys. This is an animation of the SECCHI instrument deploying.

Still from the CME animation.
Click image to view animation.

Image #3 (above): These instruments will study the 3D evolution of CME's from birth at the Sun's surface through the corona and interplanetary medium to its eventual impact on Earth. This new perspective will help us better predict where and when CME"s will arrive.



Presenter #3 - Janet Luhmann, IMPACT Principal Investigator


Still from Janet Luhmann's video
Click image to view animation.


STEREO diagram 2
Click image to enlarge.

Image #1 (above): Graphic of IMPACT instruments.

IMPACT Boom deploy
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Animation #2 (above): Boom deployment animation.

Still from animation of energy particles
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Animation #3 (above): Particle animation.



Presenter #4 - Dr. Madhulika Guhathakurta, Science Mission Directorate, NASA Headquarters


Still from Madhulika Guhathakurta's video
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NASA Heliophysics objectives

The artist's illustration highlights the fleet of Sun  

Image #1 (top): NASA's Heliophysics department objectives. Image #2 (left): The artist's illustration highlights the fleet of Sun-Earth observing spacecraft operated by NASA and its partners. STEREO data will often be used to complement other missions and vice versa. It also provides a unique service with its different perspective to space weather. Click image to enlarge. + High resolution image Credit: NASA

 
 
Rani Gran
Goddard Space Flight Center