@article{oai:nipr.repo.nii.ac.jp:00004494,
 author = {Sasaki, Sho},
 journal = {Proceedings of the NIPR Symposium on Antarctic Meteorites},
 month = {Oct},
 note = {P(論文), Implantation of the ancent solar wind is a possible noble gas source for Venus and gas-rich meteorites. During the stage of planetary accretion, dust grains re-emitted by planetesimal collisions could be targets of the solar wind implantation. The present study shows that such off-disk implantation can play an important role in noble gas capture; our results explain not only the ^<36>Ar amount in the Venusian atmosphere but also the fact that the ^<36>Ar abundance in Venus is 70 times as much as that in the Earth, assuming that gravitational scattering by the proto-Venus should enhance the orbital inclination of target materials. This mechanism may also have played a role in the origin of gas-rich meteorites.},
 pages = {326--334},
 title = {Penetration of the solar wind after dissipation of the solar nebula: Origin of Venusian Ar by off-disk implantation of the solar wind},
 volume = {2},
 year = {1989}
}