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- W4230103886 abstract "Abstract Within the recent years the spatial distribution of Zodiacal dust has been subject to a variety of modelling approaches. Whereas models derived from observations in the visual range tend to demand for an increase of interplanetary matter above the solar poles (bulges), models based on infrared measurements and extended to small r seem to favor a decrease there (holes). The models are reviewed, and the dynamical structure implicated in the models is outlined." @default.
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- W4230103886 date "1991-01-01" @default.
- W4230103886 modified "2023-09-28" @default.
- W4230103886 title "Spatial Distribution and Orbital Properties of Zodiacal Dust" @default.
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- W4230103886 doi "https://doi.org/10.1017/s0252921100066653" @default.
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