How to maintain the spatial distribution of interplanetary dust
The authors discuss two aspects related to the radial dependence of spatial density of interplanetary dust. First, they ask which spatial distribution the dust source should have to lead to the observed relative spatial distribution. Sources limited to a shell at several AU heliocentric distance are found to be inadequate, while extended (0.1 AU ≤
Leinert, C. et al.
Fecha de publicación:
2
1983