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- W2982515846 abstract "The principal scientific objective of the Solar-Terrestrial Relations Observatory (STEREO) is to understand the origin and consequences of coronal mass ejections (CMEs). CMEs are the most energetic eruptions on the Sun. They are responsible for essentially all of the largest solar energetic particle events and are the primary cause of major geomagnetic storms. They may be a critical element in the solar dynamo because they remove the dynamo-generated magnetic flux from the Sun. Two spacecraft at 1 AU from the Sun, one drifting ahead of Earth and one behind, will image CMEs. They will also map the distribution of magnetic fields and plasmas in the heliosphere and accomplish a variety of science goals described in the 1997 report of the NASA Science Definition Team for the STEREO Mission. Current plans call for the two STEREO launches in early 2003. Simultaneous image pairs will be obtained by the STEREO telescopes at gradually increasing spacecraft separations in the course of the mission. Additionally, in-situ measurements will provide accurate information about the state of the ambient solar wind and energetic particle populations ahead of and behind CMEs. These measurements will allow definitive tests of CME and interplanetary shock models. The mission will include a beacon mode to warn of either coronal or interplanetary conditions indicative of impending disturbances at Earth." @default.
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- W2982515846 date "1998-01-01" @default.
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- W2982515846 title "The Solar STEREO Mission" @default.
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