日冕凝聚区
- 网络coronal condensation
日冕凝聚区-
1983年6月11日月全食日冕凝聚区光谱分析
Analysis of the Spectra of the Coronal Condensation at the Solar Eclipse of June 11 , 1983
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本文利用势场模型，计算了1968年9月22日日面东边缘日冕凝聚区的磁场结构。
Using the potential field model , we have calculated the magnetic structure of the coronal condensation , which appeared on the east limb of the solar disk at the 22 September 1968 eclipse .
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在凝聚区旋转对称假设下，对1983年6月11日日食日冕凝聚区的光谱进行了分析处理，得到电子密度和温度在凝聚区内的分布。
The distributions of electron density and temperature in the coronal condensation were obtained by analysing the coronal spectrograms taken at the eclipse of June 11 , 1983 in Papua New Guinea .