NASA NTRS · 19830016182
Mass flow velocity distribution in the solar chromosphere
Abstract
A study of chromospheric lines (those of Si-II and Si-III) was made using the data from high resolution telescope and spectrograph (HRTS). The optically thick line profiles such as lambda 1206 due to Si-III and lambda 1265 and lambda 1533 due to Si-II were to be investigated in detail using the techniques of spectrum synthesis in an attempt to model the mass flow velocity distribution in the region of the solar atmosphere.
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Tripp, D. A.. 1981-09-30. Mass flow velocity distribution in the solar chromosphere. https://ntrs.nasa.gov/citations/19830016182
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