Sampling V-Stokes on the solar disk with Fe I 15648 Å and H Paschen β.

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Scientific paper

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Scientific paper

From exploratory observations made with a scanning spectrometer the author demonstrates that V-Stokes profiles exhibit a variety of forms. He confirms earlier work that shows the Zeeman splitting of Fe 15648 Å is complete in the magnetic fields of plage regions where field strengths of between 1000 and 2000 G can be measured. In sunspot umbrae, however, molecular blends limit the line's usefulness. Some preliminary observations with chromospheric HPβ 12818 Å are given.

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