摘要
基于我国的太阳射电宽带频谱仪(0.625～7.600GHz)在2003年10月22日～11月3日观测到8个伴生日冕物质抛射(CME)的太阳射电爆发,结合NobeyamaRadioPolarimeter(NORP)的单频观测、NobeyamaRadioheliograph(NORH)、SiberianSolarRadioTelescope(SSRT)的成像观测以及Culgoora和WAVE/WIND的低频射电频谱观测,对8个射电爆发的射电辐射特征进行了初步分析,试图从中寻找与CME伴生的射电爆发的特征。
<Abstrcat>Based on data of eight solar radio emissions associated with the coronal mass ejection (CME) in the period of October 22, 2003 to November 3, 2003 observed with the solar radio broad band spectromter of National Astronomical Observatories of China (NAOC), and combined with image data obtained from Nobeyama Radioheliograph (NoRH) and Siberian Solar Radio Telescope (SSRT), spectral data from Culgoora and Waves/Wind, and the fixed frequency data from Nobeyama Radio Polarimeter (NoRP),characteristics of radio emission of these 8 radio bursts are analyzed primaryly in order to find the relationship between the CMEs and the radio emissions.
出处
《天文研究与技术》
CSCD
北大核心
2005年第2期105-113,共9页
Astronomical Research & Technology
基金
973(G2000078403)
国家自然科学基金(No.10473020
10333030)
中国科学院2003年度"西部之光"人才培养计划支持.
