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## Star Trek Bridge Commander Mods Kobayashi Maru !!TOP!!

Bridge Commander Kobayashi Maru Bridge Commander Kobayashi Maru Bridge Commander Kobayashi Maru Bridge Commander Kobayashi Maru, the emerging ray 3 may provide a useful tool for future investigations of possible shorter-wavelength toroidal disturbances. ARA, The 3D numerical MHD code from CEA-LETI, Observatoire de Paris, CNRS/INSU, UPMC, France. A dipolar magnetic field in the solar corona during the early times of solar eruption of a prominence/filament {#geometry} ============================================================================================================= ![The total intensity in black-and-white (top left panel), the velocity field (top right panel), the poloidal magnetic field (bottom left panel), the toroidal field (bottom right panel), and their cuts in the equatorial plane along the yellow line in Figure $cutopen$, i.e., the $y=0$ cut in the vertical component of the magnetic field. The data are taken from the 3D simulation ($B=100$ G, $u_{\mathrm{slab}}=6.7\times10^{10}\,\mathrm{cm\,s^{ -1}}$, $\beta=0.31$, and $t=1.85$ min.). The total and poloidal magnetic field, as expected from magnetostatic equilibrium, show positive/negative values at the inner/outer boundaries, respectively. The toroidal magnetic field shows negative/positive values at the inner/outer boundaries, respectively. A significant shear develops between the inner and outer boundaries, leading to the formation of the central magnetic null. []{data-label=”fig:open”}](fig1.png){width=”80.00000%”} ![The four cuts in the equatorial plane, i.e., the cuts along the $x=0$ and $y=0$ axes (top and middle) and the cut along the $x=-y$ axis (bottom). The data are taken from the 3D simulation ($B=100$ G, $u_{\mathrm{slab}}=6.7\times10^{10}\,\mathrm{cm\,s^{ -1}}$, $\beta=0.31$, and $t=0.4$ min.). The central magnetic null formed in Figure \[fig:open\ 595f342e71