Abstract
The line profile of H⇓ as emanating from the interior of supergranular cells was measured at sin θ = 0, 0.6, 0.8 and 0.9. The measurements are described and the results presented.
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David, K. H.: 1961, Z. Astrophys. 53, 37
Grossmann-Doerth, U. and von Uexküll, M.: 1971, Solar Phys. 20, 31.
Grossmann-Doerth, U. and von Uexküll, M.: 1973, Solar Phys. 28, 319.
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Mitteilung aus dem Fraunhofer Institut Nr. 117.
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Grossmann-Doerth, U., Von Uexküll, M. Spectroscopic investigation of the chromosphere. Sol Phys 30, 71–74 (1973). https://doi.org/10.1007/BF00156174
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DOI: https://doi.org/10.1007/BF00156174