The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 39 Issue 1
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- Pages.73-73
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- 2014
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- 1226-2692(pISSN)
Comparison of geometrical methods to identify CME 3-D structures
- Lee, Harim (School of Space Research, Kyung Hee University) ;
- Moon, Yong-Jae (School of Space Research, Kyung Hee University) ;
- Na, Hyeonock (School of Space Research, Kyung Hee University) ;
- Jang, Soojeong (School of Space Research, Kyung Hee University)
- Published : 2014.04.10
Abstract
Several geometrical models (e.g., cone and flux rope models) have been suggested to infer 3-D parameters of CMEs using multi-view observations (STEREO/SECCHI) and single-view observations (SOHO/LASCO). To prepare for when only single view observations are available, we have made a test whether the cone model parameters from single-view observations are consistent with those from multi-view ones. For this test, we select 35 CMEs which are identified as CMEs, whose angular widths are larger than 180 degrees, by one spacecraft and as limb CMEs by the other ones. For this we use SOHO/LASCO and STEREO/SECCHI data during the period from 2010 December to 2011 July when two spacecraft were separated by
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