grid points (see also @Lander_Jones_2009; @Otani_Takahashi_Eriguchi_2009).

Numerical Results
=================

We give a brief summary of our numerical results here. First we show the basic features for negative $m$ models and the dependences of the magnetic field configurations on the values of $m$ for barotropes. We also show rotating and magnetized polytropic models in order to examine the effect of rotation on magnetic fields. The influence of the equation of state on the interior magnetic field is also displayed. We have computed $N=0.5, 1, 1.5$ polytropic models and four white dwarf models with $\rho_c = 1.0\times 10^7, 1.0 \times 10^8,$ $1.0 \times 10^9,$ and $1.0 \times 10^{10} \mathrm{g cm^{-3}}$.

Effect of the distribution of the [*toroidal*]{} current density on the distribution of the magnetic field {#Sec:current}
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   $m$    $1-q$    $H_\mathrm{c} / H_\mathrm{sur}$   ${\cal H}_p/{\cal H}$   ${\cal H}/|W|$   $\Pi/|W|$   $\alpha$   $\hat{\mu}_0$   $\hat{K}$      VC                    
  ------ -------- --------------------------------- ----------------------- ---------------- ----------- ---------- --------------- ----------- ---------- -- -- -- -- -- --
                                                                                              $N = 1.0$                                                                   
   -2.0   2.2E-2               1.03E+2                     9.987E-1             3.74E-5        3.33E-1    5.07E-2       2.28E-9       7.76E-7    5.132E-8                 
   -1.5   1.9E-3               4.44E+1                     9.982E-1             3.02E-5        3.33E-1    5.07E-2       9.65E-8       8.27E-7    2.646E-6                 
   -1.1   4.2E-4               2.19E+1                     9.978E-1             2.60E-5        3.33E-1    5.07E-2       1.80E-6       8.33E-7    2.775E-6                 
   -0.9   2.5E-4               1.62E+1                     9.976E-1             2.45E-5        3.33E-1    5.07E-2       7.74E-6       8.35E-7    2.785E-6                 
   