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