List of Tables

Table 1:
The derived solar C, N, and O abundances based on different atomic and molecular indicators using a 3D hydrodynamical model of the solar atmosphere (Asplund et al., 20042005b,aScott et al., 2006, Asplund et al., in preparation), together with the corresponding 1D results for the theoretical marcs model atmosphere (Asplund et al., 1997) and the semi-empirical model of Holweger and Müller (1974). The quoted uncertainty is only the line-to-line scatter.