*Model.* At the initial time
an explosion occurs at the point
in a region
with a magnetic field
and filled with a plasma of density
.
The explosion forms a cloud of dense plasma of radius
containing
particles .

At the initial time, the velocity of
the ions in the cloud is distributed linearly along the radius:

Here - radius vector in spherical coordinates, - is the maximum velocity of the ions in the cloud.

*Simulation example.*

Initial parameters:

, Gs | |

= | 1.00E+07 cm/s |

6.00E+18 | |

1.00E+15 | |

14.5 | |

0.83 |

See "Collisionless slowing down of nova and supernova shells in magnetized interstellar medium" for parameters definition.

Results:

B at X =0

B at Z =0

E at x = 0

E at z = 0

Cloud density at x = 0

Cloud density at z = 0

Cloud velocity at x = 0

Cloud velocity at z = 0

Background density at x = 0

Background density at z = 0

Background velocity at x = 0

Background velocity at z = 0

Bx at x = 0, T = 10, 50, 100, 140

By at x = 0, T = 10, 50, 100, 140

Bx, By, Bz at x = 0, T = 100

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