Context Navigation

← Previous Post
Next Post →

Martin's update, 6/26 '12

Disks

15au and 30au cases running.

Movies of (3d) radial inward mass flux density, $\vec{p} \cdot -\hat{r} = -(x\,p_x+y p_y+z\,p_z)/|r|$, where $\vec{p}$ is the linear momentum vector. The red material accretes while blue one goes away from the particle. Polar accretion does not dominate the toroidal+radial one.

Note that the color scale on the right is smaller than that on the left to stress gradients.

10au case http://www.pas.rochester.edu/~martinhe/2012/binary/10radFlux.gif
- 3d view of the above http://www.pas.rochester.edu/~martinhe/2012/binary/10radFlux3d.gif
20au case http://www.pas.rochester.edu/~martinhe/2012/binary/20radFlux.gif
- 3d view of the above http://www.pas.rochester.edu/~martinhe/2012/binary/20radFlux3d.gif

Paper figures page: https://clover.pas.rochester.edu/trac/astrobear/blog/martinhe06202012

New cool movie from the 10 au case (the stupid arrow should be ~1 inch to the left): http://www.pas.rochester.edu/~martinhe/2012/binary/10au-3dDisk.gif

astrobear

Context Navigation

Martin's update, 6/26 '12

Comments

Download in other formats: