Abstract
Numerical simulation based upon three‐dimensional ray‐tracing from a single source point located in the equatorial region is used to explain the wave distribution functions (WDF) found for ELF/VLF hiss detected on the GEOS satellite. Emissions at very oblique k vectors and in all azimuthal directions are shown to produce the GEOS‐1 multipeaked WDFs at the longitudes and L values close to the longitudes and L values of a chosen single source point. Inverse ray‐tracings, started with the parameters of the WDF's observed emissions, are used to locate the sources.
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