Changes between Version 18 and Version 19 of AstroBearProjects/resistiveMHD


Ignore:
Timestamp:
10/04/11 00:15:28 (13 years ago)
Author:
Shule Li
Comment:

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  • AstroBearProjects/resistiveMHD

    v18 v19  
    274274= Code Tests =
    275275= ======================= =
     276The 2-D Harris current sheet test can be set up as follows:[[BR]][[BR]]
     277[[latex($B_y(x) = b_0 tanh(x/a)$)]][[BR]][[BR]]
     278where in computational units we choose [[latex($b_0 = 1$)]] and [[latex($a = 0.5$)]].[[BR]]
     279The density profile is chosen so that the pressure equilibrium can be maintained with constant temperature.[[BR]][[BR]]
     280[[latex($\rho(x) = \rho_0/cosh^2(x/a)+\rho_c$)]][[BR]][[BR]]
     281where [[latex($\rho_0 = 1$)]] and [[latex($a = 0.5$)]]. The temperature is set to be constant as 0.5. [[BR]]
     282The domain is set to be -6.4 < x < 6.4 and -12.8< y < 12.8, with fixed resolution 480 * 960. The boundaries are all open.[[BR]]
     283The initial state is in pressure equilibrium though unstable. We put in a perturbation: [[BR]][[BR]]
     284[[latex($\B_x = B_p sin(kx)cos(ky)$)]][[BR]]
     285[[latex($\B_y = -B_p cos(kx)sin(ky)$)]][[BR]][[BR]]
     286where [[latex($\B_p$)]] is the perturbation amplitude and [[latex($k = 2\pi/L_y$)]].
     287The magnetic field and the density profiles are plotted below:[[BR]][[BR]]
     288
     289The magnetic energy is diminished at the X point which will convert to bulk ram pressure that drives the y direction outflow around the x = 0 line. [[BR]]
     290For the outflow pattern, the leading edge is bounded by intermediate shocks and the trailing edge is bounded by slow shocks. There are totally four slow mode shocks stemming from the Sweet-Parker region, as shown in the following figure.[[BR]][[BR]]
     291
     292The time evolution model can be given by the Semenov solution.[[BR]]
     293
     294
     295
     296Other possible tests:[[BR]]
    276297[[BR]][[BR]]
    277298(1) Flux Explusion Problem (Analytic 2D, resistivity only) [[BR]]