A representative set of profiles is presented for the Ca II H resonace line in Stokes V and I, for the quiet sun, plages, sunspot umbrae, and a flare, as well as one example of the Ca II K line in a sunspot penumbra. The degree of polarization is highest in the spots and zero in the quiet sun, within error limits. The V profile asymmetries are, however, highest in the flare. The spectra of the Ca II K line are used to obtain a linear relation between V(lambda) and -dI/d(lambda) and a value for B(parallel) of 820 + or - 40 G using the weak-field approximation.
CITATION STYLE
Martinez Pillet, V., Garcia Lopez, R. J., del Toro Iniesta, J. C., Rebolo, R., Vazquez, M., Beckman, J. E., & Char, S. (1990). Circular polarization of the CA II H and K lines in solar quiet and active regions. The Astrophysical Journal, 361, L81. https://doi.org/10.1086/185832
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