Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsh21a..04d&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SH21A-04
Physics
7513 Coronal Mass Ejections (2101), 7594 Instruments And Techniques, 7924 Forecasting (2722)
Scientific paper
The geometric localization technique [Pizzo and Biesecker, 2004] utilizes a series of lines of sight from two space-based observatories in order to determine gross propagation characteristics of coronal mass ejections (CMEs). This technique was developed to meet the need within the space weather community for a means to accurately determine the gross properties of Earth-directed CMEs from a near-real-time data stream, such as the one provided by the STEREO (Solar TErrestrial RElations Observatory) Space Weather Beacon. This tool works with all STEREO coronagraph observations, including COR1 and COR2. Here, we employ the geometric localization technique to the CME of 31 December 2007 and present results on the speed and direction of propagation for this CME.
Biesecker Doug A.
de Koning Curt A.
Pizzo Victor J.
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