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Associations of decimetric type Ⅲ bursts with coronal mass ejections and Hα flares
作者单位:Yuan Ma,Shuo Dai,Xue-Fei Zhang(National Astronomical Observatories of China/Yunnan Astronomical Observatory,Chinese Academy of Sciences,Kunming 650011,China);De-Yu Wang(Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China);Jun Lin(National Astronomical Observatories of China/Yunnan Astronomical Observatory,Chinese Academy of Sciences,Kunming 650011,China;Harvard-Smithsonian Center for Astrophysics,Cambridge,MA 02138,USA) 
基金项目:the Ministry of Science and Technology of China under the 973 Program,the National Natural Science Foundation of China,the Chinese Academy of Sciences under the grant 
摘    要:We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%.

关 键 词:Sun:  magnetic  fields    Sun:  flares    Sun:  radio  bursts    Sun:  coronal  mass  ejections  

Associations of decimetric type Ⅲ bursts with coronal mass ejections and Hα flares
Authors:Yuan Ma  De-Yu Wang  Jun Lin    Shuo Dai  Xue-Fei Zhang National Astronomical Observatories of China / Yunnan Astronomical Observatory  Chinese Academy of Sciences  Kunming  China Purple Mountain Observatory  Nanjing  China Harvard-Smithsonian Center for Astrophysics  Cambridge  MA  USA
Institution:Yuan Ma1,De-Yu Wang2,Jun Lin1,3,Shuo Dai1 , Xue-Fei Zhang1 1 National Astronomical Observatories of China / Yunnan Astronomical Observatory,Chinese Academy of Sciences,Kunming 650011,China 2 Purple Mountain Observatory,Nanjing 210008,China 3 Harvard-Smithsonian Center for Astrophysics,Cambridge,MA 02138,USA
Abstract:
Keywords:Sun  magnetic fields-Sun  flares-Sun  radio bursts-Sun  coronal mass ejections
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