Changes between Version 33 and Version 34 of u/erica/AccretionModelingBlog


Ignore:
Timestamp:
03/25/18 22:27:46 (8 years ago)
Author:
Erica Kaminski
Comment:

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  • u/erica/AccretionModelingBlog

    v33 v34  
    7777[[Image(press_spherical_gam1pt4.png, 35%)]]
    7878
     79A zoom-in of the pressure inside the accretion kernel with overlaid velocity vectors shows the generation of an outward traveling shock:
    7980
    8081
    81 [[Image()]]
     82[[Image(press_zoomed_gam1pt4.png, 35%)]]
     83
     84It is also notable how symmetric the pressure is within the kernel (in this plane as well as the other coordinate planes). A similar plot of density:
     85
     86[[Image(rho_zoomed_gam1pt4.png, 35%)]]
     87
     88The various profiles within the kernel seem to be identical regardless of viewing plane, until the 6th frame:
     89
     90[[Image(plane_comp_gam1pt4.png, 35%)]]
     91
     92The mass flux through a shell with $r=r_{acc}$, as well as onto the particle is much lower (and variable) than the predicted $\dot{M}$:
     93
     94[[Image(mdot_sink_gam1pt4.png, 35%)]]
     95
    8296
    8397=== 3/18/18, $\gamma=1.66$, steady-state case  ===