Abstract
AbstractExtreme ultraviolet line intensities obtained with the HCO spectrometer on Skylab are used to study the prominence-corona transition region. The spatial distributions of intensities as well as of EM are found from an almost homogeneous area in a prominence. A possible interpretation is given for the different shape of the EM curves in accordance with different models of subresolution structure.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献