Line profiles of faint Si II lines of astrophysical interest are observed in a conventional shock tube. Electron density is 1.3 × 1023 m-3, and the temperature is 11000 K. The Stark effect is the dominant broadening mechanism. The Si II line at λ 419.07 nm (multiplet 7.26, Moore 1965) Stark width is measured and compared with theoretical prediction.
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Lesage, A., & Redon, R. (2004). Stark widths of faint Si II lines. Astronomy and Astrophysics, 418(2), 765–769. https://doi.org/10.1051/0004-6361:20035585