Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh51d0298w&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SH51D-0298
Physics
5465 Rings And Dust, 5759 Rings And Dust, 6015 Dust, 6213 Dust, 2129 Interplanetary Dust
Scientific paper
The remnant magnetization of chondrite type meteorite matter indicates the existence of 10-5 - 10-3 Tesla magnetic fields in the early solar system accretion disk. Taking into account parameter regimes being typical for this early evolutionary stage of the partially ionized dusty proto-solar accretion disk we performed self-consistent three-dimensional multi fluid plasma - neutral gas - dust simulations. The results of our systematic simulations show that shear flow driven collisional interactions are able to yield self-induced magnetic fields of the order of 10-5 - 10-3 Tesla in a dusty proto-planetary accretion disk on very short time scales of the order of a few years. Thus, shear flow induced self-magnetization can yield a significant contribution to the magnetization of the early solar system and is able to explain the measured remnant magnetization of meteorite material.
No associations
LandOfFree
Self-Magnetization of the Early Solar System Matter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Self-Magnetization of the Early Solar System Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Self-Magnetization of the Early Solar System Matter will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1463155