Fractional stellar convection-zone depth and the generation of magnetic flux - an empirical approach
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[1] M. Giampapa,et al. Stellar model chromospheres. XIII. M dwarf stars. , 1982 .
[2] G. N.. IUE observations of pre-main-sequence stars. I - Mg II and Ca II resonance line fluxes for T Tauri stars , 1981 .
[3] M. Giampapa,et al. High-resolution profiles of chromospheric lines in M dwarf stars. , 1981 .
[4] E. Spiegel,et al. Magnetic activity and variations in solar luminosity , 1980, Nature.
[5] L. Cram,et al. Model chromospheres of flare stars. I - Balmer-line profiles , 1979 .
[6] J. Liebert,et al. New results from a survey of faint proper-motion stars - A probable deficiency of very low luminosity degenerates , 1979 .
[7] E. Parker. The generation of magnetic fields in astrophysical bodies. X - Magnetic buoyancy and the solar dynamo , 1975 .
[8] R. Fosbury. The Source Functions of Some Strong Lines in Late-Type Stellar Atmospheres , 1974 .
[9] Helmut A. Abt,et al. Spectral Types of M Dwarf Stars , 1974 .
[10] R. Rosner,et al. Solar magnetic fields: the generation of emerging flux , 1981 .