Abstract
We have considered the formation of Si II 1816 line in the solar chromosphere. The VAL model has been adopted as the input for the electron density and temperature. These preliminary calculations show that there are measurable changes in the profile shape of this line due to electron scattering.
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© 1991 Springer-Verlag Berlin Heidelberg
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Rangarajan, K.E., Rao, D.M. (1991). The Effects of Electron Scattering on the Si II 1816 Line in the Solar Chromosphere. In: Ulmschneider, P., Priest, E.R., Rosner, R. (eds) Mechanisms of Chromospheric and Coronal Heating. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-87455-0_15
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DOI: https://doi.org/10.1007/978-3-642-87455-0_15
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