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An empirical,statistical model for the formation of the cores of chromospheric Fraunhofer lines
Authors:Suemoto  Z
Institution:(1) Sterrewacht lsquoSonnenborghrsquo, the Astronomical Institute, Utrecht, The Netherlands
Abstract:Profiles of the Ba ii lambda 4554 resonance line and the Mg i lambda 4571 intercombination line are presented, observed near the limb of the Sun. They are obtained from eclipse spectrograms with good spectroscopic resolution and an accurate height calibration. The reduction of the observations is described and detailed profiles are given for a range of viewing angles (1/cos theta = 4 – 22).
Keywords:
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