Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp23b..01w&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SP23B-01
Physics
2111 Ejecta, Driver Gases, And Magnetic Clouds, 7513 Coronal Mass Ejections (2101), 7531 Prominence Eruptions, 7827 Kinetic And Mhd Theory
Scientific paper
Since the launch of the Solar TErrestrial RElations Observatory (STEREO), a twin spacecraft A and B, coronal mass ejections (CMEs) could be firstly seen from two angles and in a much large field of view (FOV, about 1.4 — 318 Rs) by the on board instruments Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI). Here, we report a CME rising above the west limb viewed in STEREO B but from the west solar disk in STEREO A. This CME was clearly recorded continuously in space and time by the combination of the cameras SECCHI/EUVI, COR1, COR2, HI 1 and HI 2, which make it possible to study the overall kinetic motion of the CME from its launch to beyond 1 AU. In this study, the trajectory, acceleration, velocity, and expansion of this CME throughout the FOV are analyzed.
Shen Caiming
Wang Shuang
Wang Yadong
Ye Peng
Zhang James J.
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