Physics
Scientist
Cavendish Laboratory, Cambridge.
A Study of Whistling Atmospherics at Durban
Distribution of radi-frequency brightness across the solar disk at a wavelength of 60 CM
Distribution of Radio-Frequency Brightness across the Solar Disk and the Derivation of a Model Corona
Temporal helium isotopic variations within Hawaiian volcanoes: Basalts from Mauna Loa and Haleakala
The radio "brightness" across the solar disk at a wavelength of 1.4 metres and its relation to the coronal line emission
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