Solar abundance determination from ultraviolet emission lines.
Relative solar abundance for O, Si and Fe determined from intensities of far UV emission lines of solar corona
Engineering topics
Publications and source records attributed to Goldberg, L..
Relative solar abundance for O, Si and Fe determined from intensities of far UV emission lines of solar corona
Unified theoretical model of hypersonic viscous shock layer for wide range of Reynolds numbers, including mass transfer effects
Collisional excitation of autoionizing levels in solar corona
Carbon monoxide in formation of UV solar spectrum
Collisional excitation of autoionizing levels in solar corona
Fraunhofer H and K spectral line reversals and origin in discrete transition levels
Iron abundance from faint fraunhofer lines
Design considerations of electronics system for s-16 satellite
Techniques and instrumentation for measurements of ultraviolet solar emission spectrum