Local simulations of the magnetized Kelvin-Helmholtz instability in neutron-star mergers

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Table A.6:

List of 2D merger-motivated models simulated on grids of 1024² and 2048² zones, respectively.
b₀^x [10¹³ G]	$\mathsf{M}= 1$		$\mathsf{M}= 4$
	1024²	2048²	1024²
$\pm 5$	$\surd$
10	$\surd$	$\surd$
$\pm 10$	$\surd$	$\surd$	$\surd$
20	$\surd$		$\surd$
$\pm 20$	$\surd$	$\surd$	$\surd$
40			$\surd$
$\pm 40$			$\surd$

Notes. Each simulated model is indicated by a $\surd$ sign. The initial shear profile had a maximum velocity of $v_0^x = 1.83 \times 10^{9}~$ cm/s (i.e., the Mach number of the shear flow is $\mathsf{M}= 1$ ), and a width of a = 20 m. The first column lists the initial field strength, marking models with anti-parallel initial fields by a $\pm$ preceding the numerical value. Most models were simulated using different initial perturbations, and most models were additionally simulated on coarser grids.

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