New Views of EIT Wave and CME from STEREO
On 2007 December 7, a small filament located in a small active region AR 10977 erupted and led to a B1.4 flare. An EIT wave associated with this eruption was observed both by SOHO/EIT and by EUVI on board STEREO. According to the observations from SOHO/LASCO and STEREO/COR A, we found that there was no CME associated with the EIT wave. This seems to challenge the argument that the cause of EIT waves is CME. However the data from STEREO/COR B indicated that there was a narrow CME associated with the EIT wave. This suggests that studying CMEs by investigating observations made in one direction alone may not be able to guarantee the reliability of the results.
Sun EIT waves Sun CMEs
S.Ma J.Lin P.Chen H.Chen
National Astronomical Observatories of China/Yunnan Astronomical Observatory,Chinese AcadeWy of Scie NationalAstronomical Observatories of China/Yunnan Astronomical Observatory,Chinese AcaderWy of Scie Department of Astronomy,Nanjing University,Nanjing,Jiangsu 210093,China China University of Petroleum,271 2nd North Street, Dongying,Shandong 25706l,China
国际会议
The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)
昆明
英文
57-58
2008-08-03(万方平台首次上网日期,不代表论文的发表时间)