We present a photometric and spectroscopic study of four G-K dwarfs, namely HD 166, Eri, χ 1 Ori, and κ 1 Cet. In three cases, we find a clear spatial association between photospheric and chromospheric active regions. For χ 1 Ori we do not find appreciable variations of photospheric temperature or chromospheric Hα emission. We applied a spot/plage model to the observed rotational modulation of temperature and flux to derive spot/plage parameters and to reconstruct a rough "three-dimensional" map of the outer atmosphere of κ 1 Cet, HD 166, and Eri.
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Biazzo et al. (2007) studied this question.
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