June 06, 2011
Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne
c
brown@nasa
gov
MEDIA ADVISORY: M11-112
NASA HOLDS TELECONFERENCE ABOUT CONDITIONS AT EDGE OF SOLAR SYSTEM
WASHINGTON -- NASA will host a media teleconference at 1 p m EDT on Thursday, June 9, to discuss a new computer model that shows the edge of our solar system is not smooth, but filled with a turbulent sea of magnetic bubbles
Based on Voyager data, the finding suggests we need to revise our picture of this previously unexplored region so critical for understanding how cosmic rays are created and reach near-Earth space Galactic cosmic rays are of concern for human space travel, in particular during the quiet periods called the solar minimum
The teleconference panelists are: -- Arik Posner, Voyager program scientist, Heliophysics Division, Science Mission Directorate, NASA Headquarters, Washington -- Merav Opher, assistant professor, Astronomy Department, Boston University -- James F Drake, professor of physics, University of Maryland, College Park -- Edward C Stone, Voyager project scientist, professor of physics, Caltech, Pasadena, Calif -- Eugene Parker, professor emeritus, Department of Physics, University of Chicago
To participate in the teleconference, reporters must contact Dwayne Brown at 202-358-1726 or dwayne c brown@nasa gov by 9 a m EDT on June 9 for dial-in instructions
Supporting information for the briefing will be posted at:
http://www nasa gov/sunearth
Audio of the teleconference will be streamed live on the Web at:
http://www nasa gov/newsaudio
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