Gravito-MHD of Gas-Dust Disk Near Young Sun: Dissipative Stage

Details Gravito-MHD of Gas-Dust Disk Near Young Sun: Dissipative Stage Gravito-MHD of Gas-Dust Disk Near Young Sun: Dissipative Stage

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1860v&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1860

Physics

Scientific paper

Layered models of post-accretion disk are investigated where an
accumulation of bodies occurs. At the same time, a turbulent outward
transport of an angular momentum and gas to the periphery of the disk is
accounted in the MHD-active upper layer.

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