Visualization of the Titov-Démoulin modified flux rope in COCONUT in the maximum activity solar wind. The colored lines correspond to different magnetic field lines. The seed to trace the field lines is a sphere with a radius of 0.1 R_⊙ that is placed at the positive polarity. The gray field lines are a sample of the surrounding field. The radial magnetic field at the solar surface (in Gauss) is also displayed. The flux rope is in the equatorial plane, and initially only an arc extends from the surface of the Sun.