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タイトルHalo Coronal Mass Ejections: Comparing Observations and Models
本文(外部サイト)http://hdl.handle.net/2060/20110011734
著者(英)Orlove, Matthew; SaintCyr, O.; Gopalswamy, N.; Gilbert, Holly; Mays, L.
著者所属(英)NASA Goddard Space Flight Center
発行日2011-06-12
言語eng
内容記述Since 1996, the SOHO LASCO coronagraphs have detected "halo" CMEs that appear to be directed toward Earth, but information about the size and speed of these events seen face-on has been limited. From a single vantage point along the Sun-Earth line, the primary limitation has been ambiguity in fitting the cone model (or other forward-modeling techniques, e.g., Thernisian et al., 2006). But in the past few years, the STEREO mission has provided a view of Earth-directed events from the side. These events offer the opportunity to compare measurements (width and speed) of halo CMEs observed by STEREO with models that derive halo CME properties. We report here results of such a comparison on a large sample of LASCO CMEs in the STEREO era.
NASA分類Astronomy
レポートNOGSFC.ABS.4330.2011
権利Copyright, Distribution as joint owner in the copyright


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