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A New Solar Radio Spectrometer at 1.10-2.06 GHz and First Observational Results
作者姓名:Hui-Rong Ji  Qi-Jun Pu  Yi-Hua Yan  Yu-Ying Liu  Zhi-Jun Chen  Cheng-Ming Tan  Cong-Ling Cheng  De-Bang Lao  Shu-Ke Li  Zhi-Qiang Wang  Min-Hong Yu  Jian-Nong Liu  Li-Kang Zhang and Ji-Yong Gao National Astronomical Observatories  Chinese Academy of Sciences  Beijing  Hebei Semiconductor Research Institute  Shijiazhuang
作者单位:Hui-Rong Ji,Qi-Jun Pu,Yi-Hua Yan,Yu-Ying Liu,Zhi-Jun Chen,Cheng-Ming Tan,Cong-Ling Cheng,De-Bang Lao,Shu-Ke Li,Zhi-Qiang Wang,Min-Hong Yu,Jian-Nong Liu,Li-Kang Zhang and Ji-Yong Gao National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012; Hebei Semiconductor Research Institute,Shijiazhuang 050051
基金项目:Supported by the National Natural Science Foundation of China.
摘    要:An improved Solar Radio Spectrometer working at 1.10-2.06 GHz with much improved spectral and temporal resolution, has been accomplished by the National Astronomical Observatories and Hebei Semiconductor Research Institute, based on an old spectrometer at 1-2 GHz. The new spectrometer has a spectral resolution of 4 MHz and a temporal resolution of 5ms, with an instantaneous detectable range from 0.02 to 10 times of the quiet Sun flux. It can measure both left and right circular polarization with an accuracy of 10% in degree of polarization. Some results of preliminary observations that could not be recorded by the old spectrometer at 1-2 GHz are presented.

关 键 词:太阳物理学  光谱  分光计  波长

A New Solar Radio Spectrometer at 1.10-2.06 GHz and First Observational Results
Hui-Rong Ji,Qi-Jun Pu,Yi-Hua Yan,Yu-Ying Liu,Zhi-Jun Chen,Cheng-Ming Tan,Cong-Ling Cheng,De-Bang Lao,Shu-Ke Li,Zhi-Qiang Wang,Min-Hong Yu,Jian-Nong Liu,Li-Kang Zhang and Ji-Yong Gao National Astronomical Observatories,Chinese Academy of Sciences,Beijing , Hebei Semiconductor Research Institute,Shijiazhuang .A New Solar Radio Spectrometer at 1.10-2.06 GHz and First Observational Results[J].Chinese Journal of Astronomy and Astrophysics,2005,5(4):433-441.
Authors:Hui-Rong Ji Qi-Jun Fu Yi-Hua Yan Yu-Ying Liu Zhi-Jun Chen Cheng-Ming Tan Cong-Ling Cheng De-Bang Lao Shu-Ke Li Zhi-Qiang Wang Min-Hong Yu Jian-Nong Liu Li-Kang Zhang Ji-Yong Gao
Institution:[1]National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 [2]Hebei Semiconductor Research Institute, Shijiazhuang 050051
Abstract:An improved Solar Radio Spectrometer working at 1.10-2.06 GHz with much improved spectral and temporal resolution, has been accomplished by the National Astronomical Observatories and Hebei Semiconductor Research Institute, based on an old spectrometer at 1-2 GHz. The new spectrometer has a spectral resolution of 4 MHz and a temporal resolution of 5ms, with an instantaneous detectable range from 0.02 to 10 times of the quiet Sun flux. It can measure both left and right circular polarization with an accuracy of 10% in degree of polarization. Some results of preliminary observations that could not be recorded by the old spectrometer at 1-2 GHz are presented.
Keywords:instrumentation: spectrometer - sun: radio radiation
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