The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

fig1.sav: Data for plotting Figure 1;
fig2.sav: Data for plotting Figure 2;fig3.sav: Data for plotting Figure 3;fig4.sav: Data for plotting Figure 4;fig5.sav: Data for plotting Figure 5;fig6.sav: Data for plotting Figure 6;fig7.sav: Data for plotting Figure 7;
fig8.sav: Data for plotting Figure 8;
sfig1.sav: Data for plotting Supplementary Figure 1;sfig2.sav: Data for plotting Supplementary Figure 2;sfig3.sav: Data for plotting Supplementary Figure 3;sfig4.sav: Data for plotting Supplementary Figure 4;sfig5.sav: Data for plotting Supplementary Figure 5;sfig6.sav: Data for plotting Supplementary Figure 6;sfig7.sav: Data for plotting Supplementary Figure 7;sfig8.sav: Data for plotting Supplementary Figure 8;sfig9.sav: Data for plotting Supplementary Figure 9;All files can be opened in Interactive Data Language (IDL) with command 'restore,filename'.