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  5. Near infrared spectral and polarization imaging observation of coronal emission lines during the 200

Near infrared spectral and polarization imaging observation of coronal emission lines during the 200

来源 :中国科学：物理学、力学、天文学英文版 | 被引量 : 0次 | 上传用户：wangcong1001
【摘 要】
：
During the 2008 total solar eclipse, the coronal emission lines were observed by using optical fibre spectrometric and polarization imaging system in near infra
【作 者】
：
XingMing Bao (1)  ZhiYong Zh 
【机 构】
：
1.KeyLaboratoryofSolarActivity
【出 处】
：
中国科学：物理学、力学、天文学英文版
【发表日期】
：
2009年11期
【关键词】
：
SOLAR CORONA total SOLAR ECLIPSE CORONAL emission line POLARIZATION near INFRARE 
【基金项目】
：
Supported by the National Natural Science Foundation of China (Grant No. 10843003)
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During the 2008 total solar eclipse, the coronal emission lines were observed by using optical fibre spectrometric and polarization imaging system in near infrared waveband. The profiles of the coronal emission lines including Fe XIII 10747 , 10798  and
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