Titlebook: Wave Instabilities in Space Plasmas; Proceedings of a Sym Peter J. Palmadesso,Konstantinos Papadopoulos Conference proceedings 1979 D. Reid

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Effects of Power Line Radiation into the Magnetosphere OGO-3 spectral data show evidence of enhanced chorus activity over centers of population and industry, indicating that PLR may play a significant role in the excitation of VLF whistler-mode noise and the associated precipitation of electrons. Sampled OGO-3 data showed chorus elements starting in mu

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Ariel 3 and 4 Studies of Power Line Harmonic RadiationR and associated emissions above the ionosphere and their frequency of occurrence as a function of location, intensity, storm-time, season and solar cycle..A particularly prominent zone of emission is obtained at VLF (3.2 kHz over N. America where frequent PLHR induced magnetospheric wave amplificat

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Chorus, Energetic Electrons and Magnetospheric Substormsorus, energetic (79 ± 23 keV) electron fluxes and pitch angle distributions and ambient magnetic fields obtained with OGO 5. It is found that chorus occurring within 15° of the magnetic equator (equatorial chorus) was detected during magnetospheric sub-storms and is closely related to enhanced, anis

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Chorus, Energetic Electrons and Magnetospheric Substormsorus, energetic (79 ± 23 keV) electron fluxes and pitch angle distributions and ambient magnetic fields obtained with OGO 5. It is found that chorus occurring within 15° of the magnetic equator (equatorial chorus) was detected during magnetospheric sub-storms and is closely related to enhanced, anis

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Some Theoretical Aspects of Electrostatic Double Layersnsidered. Then the time-independent double layer is discussed. The discussion deals with the potential drop, the thickness, and some necessary criteria for the existence and stability of the layer. As a complement to the study of the time-independent double layer a few remarks are also made upon the

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Magnetospheric Multiharmonic Instabilitiesron harmonic waves in a plasma consisting of a hot electron component with a loss-cone type of free energy source and a cold electron component of presumably ionospheric origin. When T./T., the ratio of cold to hot electron temperature is small, the cold upper hybrid frequency controls the harmonic

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