Version 9 (modified by 14 years ago) ( diff ) | ,
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MHD Clumps: Heterogeneity and Radiative Cooling
We seek to understand the role magnetic field alignment and clump-clump spacing (filling fraction) have on the evolution of a host of randomly-distributed clumps overrun by a steady supersonic wind.
We do so by imposing a magnetic field in two configurations: parallel (Bx) and perpendicular (By) to the shock front, both with a plasma beta value of 1. We undertake an additional case in which there is no magnetic field, for comparison. We choose two configurations of clumps: sparse and dense, which are characterized by a filling fraction,
Finally, we include the effects of radiative cooling. Based on \cite{Frank et al. 2011, Yirak et al. 2010} and references therein, we choose initial densities and temperatures such that both clump bow shocks and transmitted shocks have cooling time scales less than their respective dynamic timescales. In particular, the cloud-crushing time \citep{KMC94} given by
where
is the radius of the clump, the ratio of clump to preshock ambient density, and the shock (wind) velocity.As expected from \cite[][e.g.]{fragile2005, shin2008} and others, the Bx and hydro cases look relatively similar, while the By case is most disparate. Owing to stretching and bending of magnetic field lines, we find an amplification of field strength in _._._ of _._._. In case By, the shock speed is reduced by a factor of _._._, compared to _._._ for Bx (both relative to the hydro case).
We further discuss results below.
Note: I [Kris] am recalling the assignments below from memory so they may not be correct.
Hydro Case: Setting the Scene
Hydro sparse
Done: Brandon
Hydro dense
Done: Brandon
Bx Case: Strands Dominate
Bx sparse
Done: Shule
Bx dense
Done: Shule
By Case: Transitions to a Wall
By sparse
Jonathan: As of 12/20, needs roughly three weeks more for flow to reach edge of domain. At frame ~110 (out of an estimated 140).
{{{!comment
- Click here for a discussion on the investigation of spurious artifacts in the By case with AMR.
}}}
By dense
Erica: Restarted from beginning with fixed grid. As of 12/20, produced about 150 frames in 4 days. Here is frame 154:
Attachments (20)
- By_sparse_00154.png (94.2 KB ) - added by 14 years ago.
- density0000.png (29.3 KB ) - added by 14 years ago.
- density0001.png (59.3 KB ) - added by 14 years ago.
- By_sparse.gif (465.8 KB ) - added by 14 years ago.
- By_dense.gif (482.1 KB ) - added by 14 years ago.
- Bx_dense.gif (3.5 MB ) - added by 14 years ago.
- hydro_sparse.gif (22.1 MB ) - added by 14 years ago.
- Bx_sparse.gif (3.7 MB ) - added by 14 years ago.
- hydro_dense.gif (27.4 MB ) - added by 14 years ago.
- IO3CLLOF.png (45.5 KB ) - added by 14 years ago.
- IO3CLNoLOF.png (43.6 KB ) - added by 14 years ago.
- IO3CLLOFFixedGrid.png (36.8 KB ) - added by 14 years ago.
- IO3PLNoLOF.png (43.6 KB ) - added by 14 years ago.
- IO1CL.png (40.6 KB ) - added by 14 years ago.
- IO2CL.png (43.6 KB ) - added by 14 years ago.
- IO2CLBx.png (31.6 KB ) - added by 14 years ago.
- IO2CLHydro.png (20.5 KB ) - added by 14 years ago.
- IO2CLHydroHLLC.png (20.5 KB ) - added by 14 years ago.
- By_sparse.2.gif (8.9 MB ) - added by 14 years ago.
- rho0073.png (327.0 KB ) - added by 14 years ago.