PLUTO
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Relativistic magnetized blast wave. More...
#include "pluto.h"
Go to the source code of this file.
Functions | |
void | Init (double *us, double x1, double x2, double x3) |
void | Analysis (const Data *d, Grid *grid) |
void | UserDefBoundary (const Data *d, RBox *box, int side, Grid *grid) |
Relativistic magnetized blast wave.
Set the initial condition for the relativistic magnetized blast wave problem in 2D or 3D. It consists of a highly pressurized region inside a circle (in 2D) or a sphere (in 3D) embeddd in a static uniform medium with lower pressure. The magnetic field is constant and threads the whole computational domain.
In 3D, a linear smoothing is applied in the region . The input parameters used in this problem are:
g_inputParam[PRS_IN]
: pressure inside the initial circular (2D) or spherical (3D) region.g_inputParam[PRS_OUT]
: ambient pressureg_inputParam[RHO_OUT]
: ambient densityg_inputParam[BMAG]
: magnetic field intensityg_inputParam[THETA]
: angle between mag. field and z-axis (Cartesian only )g_inputParam[PHI]
: angle between mag. field and xy-plane (Cartesian only)g_inputParam[RADIUS]
: radius of the initial over-pressurized region.Note that a given choice of parameters can be re-scaled by an arbitrary factor by letting
.
The different configurations are:
Strongly magnetized configurations can pass this test only by taking some precautions (e.g. correcting total energy with staggered magnetic field).
Definition in file init.c.
void Init | ( | double * | us, |
double | x1, | ||
double | x2, | ||
double | x3 | ||
) |
The Init() function can be used to assign initial conditions as as a function of spatial position.
[out] | v | a pointer to a vector of primitive variables |
[in] | x1 | coordinate point in the 1st dimension |
[in] | x2 | coordinate point in the 2nd dimension |
[in] | x3 | coordinate point in the 3rdt dimension |
The meaning of x1, x2 and x3 depends on the geometry:
Variable names are accessed by means of an index v[nv], where nv = RHO is density, nv = PRS is pressure, nv = (VX1, VX2, VX3) are the three components of velocity, and so forth.
Definition at line 58 of file init.c.
Assign user-defined boundary conditions.
[in,out] | d | pointer to the PLUTO data structure containing cell-centered primitive quantities (d->Vc) and staggered magnetic fields (d->Vs, when used) to be filled. |
[in] | box | pointer to a RBox structure containing the lower and upper indices of the ghost zone-centers/nodes or edges at which data values should be assigned. |
[in] | side | specifies the boundary side where ghost zones need to be filled. It can assume the following pre-definite values: X1_BEG, X1_END, X2_BEG, X2_END, X3_BEG, X3_END. The special value side == 0 is used to control a region inside the computational domain. |
[in] | grid | pointer to an array of Grid structures. |
Assign user-defined boundary conditions in the lower boundary ghost zones. The profile is top-hat:
where and
M
is the flow Mach number (the unit velocity is the jet sound speed, so ).
Assign user-defined boundary conditions:
x < 1/6
and reflective boundary otherwise.Assign user-defined boundary conditions at inner and outer radial boundaries. Reflective conditions are applied except for the azimuthal velocity which is fixed.
Assign user-defined boundary conditions.
[in/out] | d pointer to the PLUTO data structure containing cell-centered primitive quantities (d->Vc) and staggered magnetic fields (d->Vs, when used) to be filled. | |
[in] | box | pointer to a RBox structure containing the lower and upper indices of the ghost zone-centers/nodes or edges at which data values should be assigned. |
[in] | side | specifies on which side boundary conditions need to be assigned. side can assume the following pre-definite values: X1_BEG, X1_END, X2_BEG, X2_END, X3_BEG, X3_END. The special value side == 0 is used to control a region inside the computational domain. |
[in] | grid | pointer to an array of Grid structures. |
Set the injection boundary condition at the lower z-boundary (X2-beg
must be set to userdef
in pluto.ini
). For we set constant input values (given by the GetJetValues() function while for $ R > 1 $ the solution has equatorial symmetry with respect to the
z=0
plane. To avoid numerical problems with a "top-hat" discontinuous jump, we smoothly merge the inlet and reflected value using a profile function Profile().
Provide inner radial boundary condition in polar geometry. Zero gradient is prescribed on density, pressure and magnetic field. For the velocity, zero gradient is imposed on v/r (v = vr, vphi).
The user-defined boundary is used to impose stress-free boundary and purely vertical magnetic field at the top and bottom boundaries, as done in Bodo et al. (2012). In addition, constant temperature and hydrostatic balance are imposed. For instance, at the bottom boundary, one has:
where is the value of gravity at the lower boundary. Solving for
at the bottom boundary where
gives:
where, for simplicity, we keep constant temperature in the ghost zones rather than at the boundary interface (this seems to give a more stable behavior and avoids negative densities). A similar treatment holds at the top boundary.
Assign user-defined boundary conditions. At the inner boundary we use outflow conditions, except for velocity which we reset to zero when there's an inflow