“…In the past, there seemed to be little need for a comprehensive plasmaspheric model except possibly in the study of VLF and ULF characteristics (see, for example, Carpenter and Smith [1964], Fukunishi and Lanzerotti [1974a, b]). However, as the usage of VLF and ULF for communication purposes becomes more common [Koons, 1977], and as anthropogenic VLF noise increases [Helliwell et al, 1975], there is strong evidence that the radiation belt environment [Vampola, 1977] as well as the ionosphere [Morse and Rice, 1976] may be modified by these emissions. Since the controlled transmission of VLF communication signals and the environmental impact assessment of VLF noise upon the ionosphere and magnetosphere both require comprehensive models of plasmaspheric density and composition, a physical model of the plasmasphere may perhaps be a primary requirement for such applications.…”