Radiation pressure and the composition of the solar corona.
Radiation pressure and composition of solar corona, discussing abundances of Fe, Si and Mg and transition mechanism of line absorption
Lambert, D. L.↗
Engineering topics
Publications and source records attributed to Lambert, D. L..
Radiation pressure and composition of solar corona, discussing abundances of Fe, Si and Mg and transition mechanism of line absorption
C 12/C 13 isotopic abundance ratio in solar photosphere measured with C 13 H line data, noting possible spallation process
Dissociation equilibrium of negative H ions in solar type stellar atmospheres, noting H molecule vibrational and rotational levels and continuous thermal radiation