Ion-acoustic Type Instability in Protoplanetary Disk

Details Ion-acoustic Type Instability in Protoplanetary Disk Ion-acoustic Type Instability in Protoplanetary Disk

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..703..280n&link_type=abstract

PLASMAS IN THE LABORATORY AND IN THE UNIVERSE: New Insights and New Challenges. AIP Conference Proceedings, Volume 703, pp. 280

Computer Science

Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers, Magnetohydrodynamics And Plasmas

Scientific paper

The computer simulations showed that gravitational instability
development in the two-phase medium of gas-dust circumstellar disk is
the mechanism of protoplanets formation. At the non-linear stage of
instability development, the soliton density waves of high gas density
form.

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