Some comments on Suemoto's paper 'an empirical, statistical model for the formation of the cores of chromospheric Fraunhofer lines'
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We discuss a recent model for the solar chromosphere proposed by Suemoto (Solar Phys.54, 3). We conclude that the model is incompatible with the basic constraints imposed by high resolution observations and by line formation theory, and that consequently the model does not adequately describe the solar chromosphere.
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Solar Physics