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- W1525742740 abstract "The Sun-Earth Connection Coronal and Heliospheric Investigation (SECCHI) consists of two identical telescope clusters, each having five telescopes. These telescope clusters will be mounted on the two spacecraft of the NASA STEREO Mission. They will be aimed so as to observe the Sun and the entire path from Sun to Earth. The two spacecraft will be in heliocentric orbit at approximately 1 AU, with one moving out ahead of the Earth in its annual path around the Sun; the other trailing behind the Earth. The spacecraft will be called STEREO-A (Ahead) and STEREO-B (Behin!) Over the course of a mission that is designed to last at least two years, each spacecraft will drift slowly away from the Sun-Earth line at a rate of about 22 degrees per year so that at the end of two years they will be able to see, for the first time, the plasma cloud of a coronal mass ejection (CME) from view angles separated by about 90 degrees. This will enable modeling of the three-dimensional structure of such a plasma cloud, direct measurement of its frontal velocity and volumetric expansion and, for CMEs heading toward Earth, detection and measurement of their earthward progress with greatly improved precision compared to previous coronagraphic experiments for which viewing has always been restricted to the Sun-Earth line of sight." @default.
- W1525742740 created "2016-06-24" @default.
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- W1525742740 date "2002-01-01" @default.
- W1525742740 modified "2023-09-23" @default.
- W1525742740 title "The secchi solar plasma imager for stereo" @default.
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- W1525742740 doi "https://doi.org/10.1016/s0964-2749(02)80205-0" @default.
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